From: NASA HQ
Posted: Sunday, September 2, 2012
All ISS systems continue to function nominally, except those noted previously or below. Saturday - Crew off duty.
CDR Padalka performed the routine inspection of the SM (Service Module) PSS Caution & Warning panel as part of regular Daily Morning Inspection.
Gennady also conducted the periodic checkup of the circuit breakers & fuses in the DC1 Pirs Docking Compartment. [The monthly checkup in DC1, MRM1 & MRM2 looks at AZS circuit breakers on the BVP Amp Switch Panel (they should all be On) and the LEDs (light-emitting diodes) of 14 fuses in fuse panels BPP-30 & BPP-36. MRM2 & MRM1 were derived from the DC1 concept and are very similar to it.]
FE-2 Sergei Revin serviced the BTKh-26 KASKAD experiment, extracting the top of the bioreactor (#6) from the TBU-V incubator (+29 degC), shaking it with "moderately strong" movements for 2 minutes without taking it out of the case and inserting it again in TBU-V. [Started on 8/23, this activity is being carried out for 21 days, once in the morning and once in the evening.]
Padalka, Revin, Acaba, Malenchenko, Williams & Hoshide joined in conducting the regular weekly three-hour task of thorough cleaning of their home, including all USOS (US Orbit Segment) modules like Lab, Nodes, COL (Columbus Orbital Laboratory) and Kibo JPM (JEM Pressurized Module). ["Uborka", usually done on Saturdays, includes removal of food waste products, cleaning of compartments with vacuum cleaner, damp cleaning of the SM dining table, other frequently touched surfaces and surfaces where trash is collected, as well as the sleep stations with a standard cleaning solution; also, fan screens and grilles are cleaned to avoid temperature rises. Special cleaning is also done every 90 days on the HEPA (high-efficiency particulate air) bacteria filters in the Lab.]
FE-6 Hoshide performed the regular (~weekly) inspection & maintenance, as required, of the CGBA-4 (Commercial Generic Bioprocessing Apparatus 4) and CGBA-5 payloads in their ERs (EXPRESS Racks) at Lab O2 & O1, focusing on cleaning the muffler air intakes.
FE-4 Malenchenko completed the routine daily servicing of the SOZh system (Environment Control & Life Support System, ECLSS) in the SM. [Regular daily SOZh maintenance consists, among else, of checking the ASU toilet facilities, replacement of the KTO & KBO solid waste containers, replacement of EDV-SV waste water and EDV-U urine containers and filling EDV-SV, KOV (for Elektron), EDV-ZV & EDV on RP flow regulator.]
At ~8:55am EDT, the entire crew held the regular WPC (Weekly Planning Conference) with the ground, discussing next week's "Look-Ahead Plan" (prepared jointly by MCC-H and TsUP-Moscow timeline planners), via S-band/audio, reviewing upcoming activities and any concerns about future on-orbit events.
At ~10:55am, Suni Williams powered up the SM's amateur radio equipment (Kenwood VHF transceiver with manual frequency selection, headset, & power supply) and at 11:05am conducted a ham radio session with students at the National Electronics Museum (NEM), Linthicum, MD. [NEM, located just outside Baltimore, Maryland, is home to the country's largest collection of historic defense electronics, including radar, radios, electronic countermeasures, sonar, and space sensors. The museum also has objects derived from defense electronics like the Apollo 11 camera and early GPS equipment. The students are Junior and Senior schoolers from the local Baltimore area. They have completed a six-week amateur radio course and are now licensed hams. As part of their training, they used an AMSAT satellite to make a contact. Their first contact as hams was today, with the ISS.]
At ~12:00pm, Sunita Williams had her weekly PFC (Private Family Conference), via S-band/audio and Ku-band/MS-NetMeeting application (which displays the uplinked ground video on an SSC laptop).
The crew worked out on the CEVIS cycle ergometer with vibration stabilization (FE-5, FE-6), TVIS treadmill with vibration isolation & stabilization (CDR, FE-2/2x, FE-3, FE-4), ARED advanced resistive exercise device (CDR, FE-3, FE-5, FE-6), and VELO ergometer bike with load trainer (FE-4) [FE-6 & FE-5 are on the special experimental SPRINT protocol which diverts from the regular 2.5 hrs per day exercise regime and introduces special daily sessions involving resistive and aerobic (interval & continuous) exercise, followed by a USND (Ultrasound) leg muscle self scan in COL. No exercise is being timelined for Friday. If any day is not completed, Suni & Aki pick up where they left off, i.e., they would be finishing out the week with the last day of exercise on her off day. Suni's protocol for today was on ARED/CEVIS (continuous), with CEVIS (interval, 2 min.), ARED/CEVIS (cont.), CEVIS (int., 30 s.), ARED/T2 or CEVIS (cont.), T2 or CEVIS (int., 4 m.) & T2 Kinematics for the next 6 days. Aki's protocol for today showed CEVIS (interval, 2 min.), ARED/CEVIS (aerobic, cont.), CEVIS (int. 30 sec), ARED/CEVIS & T2 or CEVIS (int., 4 min.) for the next 4 days.]
Before his first exercise run on the TVIS treadmill, Joe Acaba observed Yuri Malenchenko's workout on the machine and then formatted a PCMCIA (Portable Computer Memory Card International Adapter) memory card for his own TVIS exercise program.
Due to power limitations with the current 3-MBSU jumper configuration, T2/COLBERT has been powered down because it is a big power draw on Channel 4. For the time being, T2 sessions have been rescheduled as CEVIS for Suni, Aki & Joe, and TVIS for Gennady.
Tasks listed for Revin, Malenchenko & Padalka on the Russian discretionary "time permitting" job for today were -
. More preparation & downlinking of reportages (written text, photos, videos) for the Roskosmos website to promote Russia's manned space program (max. file size 500 Mb), and
. A detailed & general view photo session with TEKh-52 Vizir of the flooding which occurred overnight on 8/21-22 at the Black Sea; [the disaster zone includes the towns Novomikhalovsky, Lermontovo and Tenginka, the Shapsukho & Nechepsukho river valleys and the adjacent mountain region. Novomikhalovsky is located on the Tuapse-Novorossiisk Highway, 33 km from Tuapse and 14 km from Dzubgi. The town is situated in the Nechepsukho river valley and its tributary Psebe, where Nechepsukho is falling into Mikhalovsky Bay in the Black Sea. As a result of torrential rain the Nechepsukho River flooded. 600 houses, a hospital and a school were in the disaster zone. Four people died, 1500 were affected, including 275 children. Municipal infrastructures need to be restored. Lermontovo is located on the shores of Tenginsky Bay of the Black Sea, at the inflow of Shapsukho River. The valley of that river is approx. 40 km in length, 5 km to the east of Dzubgi on the Tuapse-Novorosskiisk highway and 55 km from Tuapse. The Tenginka village is located 4 km upriver], and
. Recording high-resolution video with the SONY HVR-Z7E to be used in a joint project of Roskosmos TV Studio with Karusel (Carousel) TV Channel for children ages 8 to 12 years, the "It's Time to go to space!" program, which has a segment where Russian cosmonauts are discussing their work &, answer viewers' questions; the footage was then to be downlinked to TsUP-Moscow.
MBSU1 Update: With the current configuration, ISS is in a stable but non-optimal power configuration. MCC-H flight controllers are managing the loads and making adjustments as necessary for specific requests. A second spacewalk, EVA-19, is being planned for as early as Tuesday, 9/4, to attempt to install & connect MBSU1. SSRMS (Space Station Remote Manipulator System) capability is required for the MBSU translations, but there will not be a certified SSRMS operator on board after Soyuz 30S departure (9/16) and prior to 32S arrival (10/17). Hardware teams are working to determine what caused the failure and propose alternate methods, including assessing any additional available tools, to seat the MBSU bolts. The crew has a full day off today and will start EVA preps tomorrow (Sunday), with procedure review, conferences & suit checks, with final procedure review and tool configuration on Monday (U.S. Labor Day). Post-EVA events will be replanned as required. Due to issues with cooling loop temperatures in Aki's EMU (Extravehicular Mobility Unit) on 8/30, the suit was declared NoGo, and Suni & Aki resized replacement suits yesterday: Suni will be using a large-size EMU adjusted to "medium size", and Aki will don the medium-size EMU Suni used on EVA-18. Also, NASA has asked JAXA to evaluate a delay of HTV3 (H-II Transfer Vehicle 3) unberthing until the week of 9/16 to relieve the onboard timeline.
ISS Orbit (as of this morning, 9:48am EDT [= epoch])
Mean altitude -- 416.0 km
Apogee height -- 426.5 km
Perigee height -- 405.5 km
Period -- 92.89 min.
Inclination (to Equator) -- 51.65 deg
Eccentricity -- 0.0015435
Solar Beta Angle -- -34.1 deg (magnitude increasing)
Orbits per 24-hr. day -- 15.50
Mean altitude loss in the last 24 hours -- 104 m
Revolutions since FGB/Zarya launch (Nov. 98) -- 78,989
Time in orbit (station) -- 5034 days
Time in orbit (crews, cum.) -- 4321 days.
Weekly Science Update (Expedition Thirty-Two - Week 9).
2D NANO Template (JAXA): Mission completed.
3D SPACE: Complete.
ACE-1 (Advanced Colloids Experiment 1, NASA): No report.
ALTCRISS (Alteino Long Term monitoring of Cosmic Rays on the ISS): Complete.
ALTEA SHIELD Shielding (NASA/ASI): At the time of reporting (8/30), the session #2 has progressed nominally, with 21 cumulative days of science acquisition. Also for the second measurement session, the minimum duration is 40 days, preferred duration 60 days. [Cosmic radiation consists of very small, atomic-sized particles that are flying around in space at tremendous speeds. Their energy is so high that these particles, like tiny bullets, can permeate through the complete structure of the ISS. Exposure of astronauts to cosmic radiation is risky from a medical point of view. The best way to protect our astronauts against cosmic radiation is to build the complete ISS from lead! This would solve the problem but the enormous mass can impossibly be launched into space. Therefore different materials, much lighter than lead, are being tested to be used as shielding materials. Two of those will be investigated in the ALTEA-SHIELD experiment. The effectiveness of the shielding materials will be measured on board by a set of special radiation detectors. Some detectors will be covered with tiles made of shielding materials, some others will not. We are looking forward to find out what difference it will make!"]
Amine Swingbed (NASA): No report.
AMS-02 (Alpha Magnetic Spectrometer): No report.
APEX (Advanced Plant Experiments on Orbit) -Cambium: No report.
APEX-TAGES (Transgenic Arabidopsis Gene Expression System): No report.
Asian Seed 2010 (JAXA): Returned on ULF6.
BASS (Burning and Suppression of Solids, NASA): (The BASS hardware has been stowed until we resume tests beginning sometime in December 2012 or January 2013.)
BCAT-6 (Binary Colloidal Alloy Test 6, CSA): No report. [Colloids are particles as small as a few tens of nanometers (a thousandth of a thousandth of a millimeter) that are suspended in a medium, usually a liquid or a gas. The name "colloid" comes from the Greek word for "glue", and expresses very important properties of colloids: when small and light enough, particles can be influenced in their behavior by forces of electromagnetic origin, and make them stick together, or repel each other depending on the configuration. Colloids are widely studied in science because the forces between particles can be controlled and tuned and because particles, while being small enough to be influenced by such forces, are big and slow enough to be seen with a relatively simple and inexpensive laboratory instrument like a microscope. This is why colloids are often studied as model for molecular systems (like standard gases or liquids) where molecules, the individual constituents, are much smaller than colloids and cannot be seen with light. As mentioned, forces between colloids can be tuned giving rise to a rich variety of phenomena. One of them is aggregation, which is when particles stick together and tend to form structures. Among the many ways to induce particle aggregation, one allows to do so by controlling the temperature of the solution in which the particles are immersed, thanks to very weak forces called "critical Casimir forces" that have been predicted more than 30 years ago but just partially verified in experiments. The objective of SODI COLLOID is to measure such forces and produce a controlled aggregation of tiny plastic particles. This would allow to shed light on critical Casimir forces and to make a step towards the fabrication of new nanostructured materials with remarkable optical properties for industrial applications.]
BCAT-C1 (Binary Colloidal Alloy Test C1, CSA): No report.
BLB (Biolab, ESA): No report.
BIORHYTHMS 48 (Biological Rhythms, JAXA): No report.
BISE (Bodies in the Space Environment, CSA): No report.
BISPHOSPHONATES: No report.
BXF-Facility (Boiling eXperiment Facility, NASA): No report.
BXF-MABE (Microheater Array Boiling Experiment, NASA): No report.
BXF-NPBX (Pool Boiling Experiment, NASA): No report.
CARD (Long Term Microgravity Model for Investigating Mechanisms of Heart Disease, ESA): No report.
CB (JAXA Clean Bench): No report.
CBEF-2 (JAXA Cell Biology Experiment Facility)/SPACE SEED: No report.
CCISS (Cardiovascular & Cerebrovascular Control on Return from ISS): No report.
CERISE (JAXA): No report.
CCF (Capillary Channel Flow, NASA): No report.
CFE-2 (Capillary Flow Experiment 2, NASA): No report.
CFS-A (Colored Fungi in Space-A, ESA): No report.
CSI-5/CGBA-5 (CGBA Science Insert #5/Commercial Generic Bioprocessing Apparatus 5): No report.
CGBA-2 (Commercial Generic Bioprocessing Apparatus 2): Complete.
CIR (Combustion Integrated Rack), MDCA/Flex: No report.
CIRCADIAN RHYTHMS (ESA): No report.
Commercial (Inc 23&24, JAXA): No report.
Commercial (Inc 25 & 26, JAXA): No report.
Commercial (Inc 32, JAXA): Aki, thank you very much for your attractive actions, all of the video taken was downlinked successfully on 8/29. We can hardly wait for the CM (Commercial Mission) to be aired.
CSAC (Chip-Scale Atomic Clock, SPHERES): No report.
CSLM-2 (Coarsening in Solid-Liquid Mixtures 2): No report.
CsPins (JAXA): No report.
CubeLab: No report.
CW/CR (Cell Wall/Resist Wall) in EMCS (European Modular Cultivation System): Complete.
DECLIC-ALI (Device for the Study of Critical Liquids & Crystallization-ALICE-like, CNES/NASA): No report.
DomeGene (JAXA): Complete.
DOSIS (Dose Distribution Inside ISS, ESA): Nominal science acquisition with active and passive dosimeters inside Columbus.
DTN (Delay Tolerant Network, NASA): "Thank you, Sunita, for your work on setting up the DTN-Laptop in Columbus. We were able to verify via CGBA-5 that the connection was successful. The ER2 RIC has an old software load which will not support DTN activities, and will need to be updated. We will begin commissioning activities from the ground once this update is completed."
EarthKAM (Earth Knowledge Acquired by Middle School Students): No report.
EDR (European Drawer Rack, ESA): Activated on 8/23 to support the ERB-2 index file transfer activity.
EKE (Endurance Capacity by Gas Exchange and Heart Rate Kinetics During Physical Training, ESA): No report.
ELITE-S2 (Elaboratore Immagini Televisive - Space 2): Planned.
EMCS (European Modular Cultivation System): No report.
ENERGY (ESA): No report. [Background: In the ENERGY experiment, astronauts are invited to participate in a study that aimed to evaluate how much food is needed for astronauts during long-term space missions. To do so, the science team will measure every component or variable of the astronaut's energy expenditure reflecting his energy needs. Those variables will be measured twice: up to 4 months before flight and after at least 3 months in space but 3 weeks before landing. The changes in the astronaut's energy balance and expenditure will be measured, which will help in deriving an equation for energy requirements in weightlessness. This will contribute to planning adequate, but not excessive cargo supplies for food.]
ENose (Electronic Nose): No report.
EPM (European Physiology Module): No report.
EPO (Education Payload Operations, NASA) Demos: "Suni, thank you for completing the EPO Exploration Design Challenge Demo. The video will be used to launch an engineering design contest related to the anticipated Orion mission and the challenge of radiation protection. The video will also be edited and posted to an upcoming NASA education website highlighting space life sciences."
EPO (Educational Payload Operations, NASA) (Eye in the Sky; Sleep 2): No report.
EPO (Educational Payload Operations, NASA) (Sesame Street): No report.
EPO (Educational Payload Operations, NASA) (Kids in Micro-G): No report.
EPO (Educational Payload Operations, NASA) (Earth/Moon/Mars Demo): No report.
EPO (Educational Payload Operations, NASA) (Space Sports): No report.
EPO (Educational Payload Operations, NASA) (ISS Orbit): No report.
EPO (Educational Payload Operations, ESA): No report.
EPO CONVECTIONS (ESA): "No report.
EPO MISSION X (ESA): No report.
EPO Spaceship Earth (ESA): No report.
EPO LES-2 (ESA): No report.
EPO GREENHOUSE (ESA): No report.
EPO 3-min Video (JAXA): No report.
EPO J-Astro Report (JAXA): No report.
EPO Dewey's Forest (JAXA): Closed out on 3/15.
EPO Space Clothes (JAXA): Complete.
EPO Hiten (Dance, JAXA): No report.
EPO Lego Bricks (NASA, JAXA): No report.
EPO Moon Score (JAXA): No report.
EPO OpticSphere & ISSOrbit-Demo (NASA): No report.
EPO Kibo Kids Tour (JAXA): Complete.
EPO Paper Craft (Origami, JAXA): No report.
EPO Poem (JAXA): No report.
EPO-5 SpaceBottle (Message in a Bottle, JAXA): No report.
EPO-6 Spiral Top 2 (JAXA): No report.
EPO-7 Doctor Demo (JAXA): No report.
EPO-7 Green Tea Preparation (JAXA): No report.
EPO-7 Ink Ball (JAXA): No report.
EPO-7 Video (JAXA): EPO-7 Try Zero-G (JAXA): No report.
EPO-8 Space Sakura (JAXA): No report.
EPO-8 Space Musical Instruments (JAXA): No report.
EPO-9 (JAXA): "Aki, thank you for JAXA Report04 completion on 8/19G."
ERB-2 (Erasmus Recording Binocular, ESA): [ERB-2 aims are to develop narrated video material for various PR & educational products & events, including a 3D interior station view.] No report.
ETD (Eye Tracking Device): Completed.
FACET-2 (JAXA): No report.
FERULATE (JAXA): No report.
FIR/LMM/CVB (Fluids Integrated Rack / Light Microscopy Module / Constrained Vapor Bubble): No report.
Fish Scales (JAXA): Completed on FD7/ULF-4 and returned on STS-132.
FOAM STABILITY EPO (ESA): No report.
FOCUS: No report.
FSL (Fluid Science Laboratory, ESA): No report.
FWED (Flywheel Exercise Device, ESA): No report.
GENARA-A (Gravity Regulated Genes in Arabidopsis A/ESA): No report.
GEOFLOW-2 (ESA): Experiment completed! [Background: Everybody is familiar with liquids. In an average day we get to use, handle or drink water or other liquids. And everybody knows how fluids (that is liquids and gases) behave: when subjected to a net force, may be pressure, a temperature difference or gravity, they can move freely. Scientists have been studying how fluids move for centuries, and managed to write mathematical formulas that can describe and predict such movements. Unfortunately, these equations are extremely complex and only approximate solutions are known. As a result, our quantitative understanding of fluid movement is just partial. This is especially true for natural phenomena where the forces can be enormous and unpredictable, like in oceans or in the atmosphere, or the interior of the earth, where rocks are exposed to pressures and temperatures so incredibly high that they slowly move and adapt their shape. That is, over hundreds of years rocks flow just like a very viscous liquid. Scientists try to study such flows but cannot observe them directly due to the fact that they take place deep beneath the surface of our planet. The only way is to have computers simulating those movements starting from the equations, but how to check whether computers are correct? This is what Geoflow II is trying to answer on board the International Space Station. Geoflow II is a miniature planet that has some of its essential ingredients: a fluid can freely move inside a spherical container that rotates, has temperature differences and has a simulated gravity directed towards the centre just like in a real planet. By taking pictures of the fluid movements, scientists are able to understand the essential characteristics of the flows and determine whether computer simulations are correct or whether they need to be refined and improved towards a better understanding of the elusive movements that take place inside our planet.]
GLACIER (General Laboratory Active Cryogenic ISS Experiment Refrigerator, NASA): "Thank you for your work this week on the battery and desiccant replacement."
HAIR (JAXA): "Aki, thank you for your first hair sampling and your CrewNote input."
HDTV System (JAXA): No report.
Hicari (JAXA): No report.
Holter ECG (JAXA): No report.
HQPC (JAXA): No report.
HREP (HICO/Hyperspectral Imager for the Coastal Ocean & RAIDS/Remote Atmospheric & Ionospheric Detection System/JAXA): HICO has taken 6291 images to-date. The most recent HICO images include Tokyo Bay, the coast of Italy near Venice, a couple of lakes in Oregon and part of the coast of Australia. RAIDS is continuing to collect secondary Science data including nighttime atmospheric disk photometry, spectra and temperatures. Extreme Ultra Violet airglow spectroscopy and optical contamination studies will also be performed.
HRF-1 (Human Research Facility 1, NASA): No report.
HydroTropi (Hydrotropism & Auxin-Inducible Gene Expression in Roots Grown under Microgravity Conditions/JAXA): No report.
ICE CRYSTAL (JAXA): Complete.
ICV (Integrated Cardiovascular): "Aki, we've received your FD30 Ambulatory Monitoring data on the ground, and have been able to confirm the expected file quantity and sizes. Thank you! A brief review of the Actiwatch data revealed an occasional activity count during the time between watch doff/stow in the Holter Kit and download; this does not impact the data you collected, but rather is a preliminary indication that the batteries may be starting to run low. As a result, we will be sending you to a new set of watches during your next session (~FD75)."
IMMUNO (Neuroendocrine & Immune Responses in Humans During & After Long Term Stay at ISS): No report.
INTEGRATED IMMUNE: No report.
InSPACE-3 (Investigating the Structure of Paramagnetic Aggregates from Colloidal Emulsions 3): "Suni: Thank you very much for doing the InSPACE hardware install, and especially working through diagnosing what was wrong with the camera giving the pitch black background. We were so happy it wasn't the green LED light source(s), as we don't have any spares! But thanks to your very astute observation, it was a misalignment of the lens assembly and you were able to successfully realign it. Thanks for your willingness to go back and finish it up for the afternoon. Looking forward to starting our science ops when time permits."
IRIS (Image Reversal in Space, CSA): No report.
ISS Amateur/Ham Radio: Three contacts were made this week. The total number of contacts for Inc 31-32 is now up to 21.
ISSAC (ISS Agricultural Camera, NASA): "ISSAC Imaging operations are nominal and on-going. Special thanks to Joe, Suni, and Aki for their help and support in opening the lab window shutter in spite of their busy schedule. From 7/27 to 8/29, the crew opened the shutter 44 out of 60 times that we requested. Due to which ISSAC was able to collect ~58 target strips (equivalent to ~2500 images). Kudos to everyone!"
IV Gen (Intravenous Fluids Generation): No report.
JOURNALS (Behavioral Issues Associated with Isolation and Confinement, NASA): No report. [Studies conducted on Earth have shown that analyzing the content of journals and diaries is an effective method for identifying the issues that are most important to a person. The method is based on the reasonable assumption that the frequency that an issue or category of issues is mentioned in a journal reflects the importance of that issue or category to the writer. The tone of each entry (positive, negative, or neutral) and phase of the expedition also are variables of interest. Study results will lead to recommendations for the design of equipment, facilities, procedures, and training to help sustain behavioral adjustment and performance during long-duration space expeditions to the ISS, asteroids, the Moon, Mars, and beyond. Results from this study could help to improve the behavioral performance of people living and working under a variety of conditions here on Earth.]
KUBIK 3/6, KID (ESA): No report.
LMM/PACE-2 (Light Microscopy Module / Preliminary Advanced Colloids Experiment): No report.
LEGO Bricks: "Suni: Thank you for performing the Spinner activity. Future robotic model experiments are planned."
LOCAD-PTS (Lab-on-a-Chip Application Development-Portable Test System): No report.
MAMS (Microgravity Acceleration Measurement System, NASA): No report.
Marangoni Exp. (JAXA): No report.
Marangoni DSD - Dynamic Surf (JAXA): Payload name was change from Marangoni DSD to Dynamic Surf.
Marangoni UVP (JAXA): No report.
MARES (Muscle Atrophy Research & Exercise System, ESA/NASA): No report.
Matryoshka-2 (RSA): No report.
MAXI (Monitor of All-sky X-ray Image, JAXA): No report.
MCE (Multi-Mission Consolidated Equipment, JAXA): The ground team successfully completed deployment of the Inflatable Material experimental Plate (IMP) on 8/24. The team continues REX-J checkout and commanding this week.
MDCA/Flex-2: On 8/27-8/28, we performed the first MDCA/FLEX-2 Convective Flow test points. We successfully ran these test points using the Location 2 fuel pathway, so it appears that replacing the MDCA Needle 2 resolved the obstruction issue with the Location 2 fuel pathway. This is good news! The MDCA Fuel Reservoir installed in Location 2 still has a good amount of decane fuel, which could have been potentially unusable if the obstruction was in the reservoir assembly.
MEIS (Marangoni Experiment for ISS) in JAXA FPEF (Fluid Physics Experiment Facility): No report.
MELFI (Minus Eighty Laboratory Freezer for ISS, NASA): No report.
Microbe-3 (JAXA): "Aki, thank you very much for the dust sampling around JEM on 8/28."
Micro-G Clay (JAXA EPO): Complete.
Miscible Fluids in Microgravity (MFMG): No report.
MISSE-8 (Materials ISS Experiment 8): MISSE-8 is nominal. PASCAL is performing nominal commanding that produced IV curves of the solar cells. IV curves are plots of the current versus voltage for solar cells and tell a lot about how these are performing. The SpaceCube experiment is running code for new radiation hardening by software.
MMA (JAXA/Microgravity Measurement Apparatus): No report.
MPAC/SEED (JAXA): No report.
MSG (Microgravity Science Glovebox, NASA): No report.
MSG-SAME (Microgravity Science Glovebox -Smoke Aerosol Measurement Experiment): No report.
MSPR (Multi Purpose Small Payload Rack, JAXA): No report.
MSL (Materials Science Laboratory, ESA): Three processed Sample Cartridge Assemblies (SCA's) have been returned with SpX-D.
MTR-2 (Russian radiation measurements): Passive dosimeters measurements in DC-1 "Pirs".
MYCO 3 (JAXA): On 9/22, Mike and Satoshi completed sample collection.
MyoLab (JAXA): Completed on 4/20.
NanoRacks (NASA): No report.
NANOSKELETON (Production of High Performance Nanomaterials in Microgravity, JAXA): No report.
NANO STEP (JAXA): The ground team has been continuing to observe protein crystal growth, now in phase 3 for 12 days duration. This run #1 will continue until 9/7. The AAA rotation speed change on 8/23, and the MTL Ryutai flow rate change on 8/28 didn't let us find any obvious change in the unstable interferometer fringe.
NEURORAD (JAXA): No report.
NEUROSPAT (ESA/Study of Spatial Cognition, Novelty Processing and Sensorimotor Integration): No report. [During microgravity stay, the human body goes through multitude of physiological changes in order to accommodate to the new environment. As the brain is a master organ where major crucial processes take place, it is fundamental to understand how it manages adaptation for living in Space. One of the main purposes of Neurospat (NES) experiment is to focus on how microgravity environment influences cerebral activity of astronauts aboard ISS. For this, the global electrical activity of the brain of the astronaut is measured thanks to electroencephalogram (EEG) technique, while he or she is executing specific tasks through a computer as if it was a kind of videogame. In practice, the astronaut is wearing a specially equipped cap with passive, gel filled electrodes that are in contact with his/her scalp while he or she is performing the specific tasks that we have designed. These are visual-orientation perception and visuo-motor tracking tasks that may be encountered on a daily basis. The tasks allow the study of 5 cognitive processes: Perception, Attention, Memorization, Decision and Action. Besides there are also task-irrelevant images that are showed to the astronaut in order to assess how well he or she processes novel visual stimuli. The electrodes all over the scalp are linked to sensitive amplifiers that allow us to measure small variations of electrical potential between different regions of the scalp. These signals are in turn used to estimate activity in the cerebral cortex related to the task being performed. Also, they serve to identify the mental processes associated with these tasks and to localize in the brain the sources of the underlying neural activity. After analysis of the data we can better understand whether the novel environment of microgravity accompanied by a multitude of stressors may place an increased load on the cognitive capacity of the human brain and whether the sensory signals and motor responses of astronauts are processed and interpreted differently because a new reference frame.]
NightPod (ESA): NightPod images have been presented in a news blog on the ESA PromISSe website: http://blogs.esa.int/promisse/2012/04/05/nightpod/
NOA-1/-2 (Nitric Oxide Analyzer, ESA): Complete.
NUTRITION w/REPOSITORY/ProK: No report.
ODK-2 (Onboard Diagnostic Kit 2, JAXA): No report.
PADIAC (Pathway Different Activators, ESA): No report.
PADLES (JAXA, Area PADLES 6/7; Passive Area Dosimeter for Lifescience Experiment in Space): The 17 dosimeters installed inside the JEM continue to acquire radiation data. This experiment will continue until 30S return.
PASSAGES (JAXA): No report. [PASSAGES is an experiment about the strategies involved in the perception of the world around us. Seeing correctly the world is necessary to success our gestures, our actions, such as catching a ball, stepping an obstacle on the ground or passing through an opened door. In this experiment, we want to know if the strategies involved on Earth continue to be used when the astronaut is in a weightlessness environment for a long period. To investigate this question, the participant sees 3D scenes on the screen of a laptop such as a video game. The scene is a room with an opening which can vary in width. The task of the participant is to decide if yes or no he or she could pass through the aperture without rotating or scrunching the shoulders. The science team uses typical methods from psychophysics and manipulates several factors to highlight the strategies used by the participant. Then, the science team will compare the performances obtained on ground with those obtained onboard.]
PCDF-PU (Protein Crystallization Diagnostic Facility - Process Unit): No report.
PCG (JAXA, Protein Crystal Growth): Mission completed last week.
PCRF (Protein Crystallization Research Facility) Reconfiguration (JAXA): See PCG.
PLSG (Plant Signaling, NASA/ESA): No report.
PMDIS (Perceptual Motor Deficits in Space): Complete.
POLCA/GRAVIGEN (ESA): Complete.
Portable PFS: Used for Suni's first VO2max session. Refer to VO2max / EKE / THERMOLAB.
Pro K: No report.
RadGene & LOH (JAXA): Complete.
RadSilk (JAXA): No report.
Reaction Self Test (RST/Psychomotor Vigilance Self Test on the ISS): "Joe, Suni, and Aki, thank you for your participation in Reaction Self Test! Your continued efforts through normal, sleep shift, and EVA sessions are greatly appreciated!"
Reversible Figures (ESA): No report. [Background: The objective of this study is to understand the relationship between gravity and depth perception. Another objective is to identify the problems associated with depth and distance perception in astronauts with the goal of developing countermeasures to reduce any associated performance alteration. This experiment investigates cases in which what astronauts might think to see, fails to achieve a correct representation of the environment, namely, optical illusions. Ten ambiguous figures, with or without depth cues, are presented to an astronaut in virtual reality goggles. These figures are ambiguous because they can be seen at first sight in two different ways. The figure does not change, but after some time the brain reverses (flip-flops) its interpretation. The astronaut is asked to look closely at each figure and to indicate with a mouse trackball which view he/she sees first, and when the view flip-flops. The interval between the views will be compared between 1g and 0g conditions. In 0g, the astronaut will do the test while free-floating to eliminate all orientation cues. This experiment will be performed three times pre-flight, then up to six times in-flight, and again three times post-flight. The science team will then compare the results of these tests across these gravitational environments. It is expected that the frequency of flip-flops of figures with depth cues will be different in between 0g and 1g, and that an adaptation to long-term exposure to weightlessness, as well as a re-adaptation to Earth gravity, will take place.]
ROALD-2 (Role of Apoptosis in Lymphocyte Depression 2, ESA): No report. [Background: The ROALD-2 experiment studies how the function of T-cells from the immune system are affected by microgravity and spaceflight. T-cells play an important role in controlling the immune systems response to infection. It has previously been shown that the immune response of astronauts can be reduced following spaceflight and it has also been shown that the activation of T-cells in culture is reduced in microgravity. A series of experiments on T-cells and other immune system cells have been previously performed by different scientific teams on Space Shuttle and the ISS over the last 30 years. The data from these individual experiments provides information which together can be used to understand the mechanisms by which gravity or the absence of gravity can affect T-cell function.]
Robonaut (NASA): Robonaut worked with Task Panels C and D for the first time this week. On 8/27, Robonaut calibrated the location of Task Panel C. It then located, grasped, and seized the handrail on Panel C through some automated scripts and minor adjustment from the R2 Ops team. On 8/28, in addition to repeating the tasks of the previous day, Robonaut removed a cleaning wipe from a package mounted to Task Panel D and proceeded to wipe the exterior face of the handrail on Panel C with manual and automated commanding. All but two of the faults Robonaut annunciated were cleared from the ground, with minimal crew interaction being required to clear the other two. The R2 Ops team will be using lessons learned from this two day session to build more robust and automated activities.
RYUTAI Rack (JAXA): No report.
SAIBO Rack (JAXA): No report.
SAMS/MAMS (Space & Microgravity Acceleration Measurement Systems): No report.
SAMPLE: Complete. SCaN (Space Communications and Navigation Testbed, NASA): No report. [Background: The SCaN Testbed provides an orbiting laboratory on space station for the development of SDR (Software Defined Radio) technology. These systems will allow researchers to conduct a suite of experiments over the next several years, enabling the advancement of a new generation of space communications. The testbed is the first space hardware to provide an experimental laboratory to demonstrate many new capabilities, including new communications, networking and navigation techniques that utilize SDR technology. The SCaN Testbed includes three such radio devices, each with different capabilities. These devices will be used by researchers to advance this technology over the Testbed's five year planned life in orbit. Two SDRs were developed under cooperative agreements with General Dynamics and Harris Corp., and the third was developed by NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif. JPL also provided the five-antenna system on the exterior of the testbed, used to communicate with NASA's orbiting communications relay satellites and NASA ground stations across the United States.]
SCOF (Solution Crystallization Observation Facility, JAXA): No report.
SEDA-AP (Space Environment Data Acquisition Equipment-Attached Payload, JAXA): Continuing telemetry monitoring.
SHD (Space Headaches, ESA): "Dear Joe, many thanks for your continuous support in filling your weekly questionnaires, much appreciated! (2 more to go ;-))". [Background: The neurologists from Leiden University want to study the question whether the astronauts, while in space, suffer from the headaches. With the help of simple questionnaires the astronauts will register the headache episodes and the eventual accompanying symptoms. The results will hopefully help to characterize the frequency and characteristics of space headache and to develop countermeasure to prevent/minimize headache occurrence during the space flight.]
SHERE II (Shear History Extensional Rheology Experiment II): No report.
SLAMMD (Space Linear Acceleration Mass Measurement Device): No report.
SLEEP (Sleep-Wake Actigraphy & Light Exposure during Spaceflight): No report.
SLICE (Structure & Liftoff In Combustion Experiment): No report. [See under BASS.]
SMILES (JAXA): Continuing telemetry monitoring.
SODI/IVIDIL (Selectable Optical Diagnostics Instrument/Influence of Vibration on Diffusion in Liquids, ESA): No report.
SODI/COLLOID (Selectable Optical Diagnostics Instrument/Colloid): No report.
SODI-DSC (Selectable Optical Diagnostics Instrument/Diffusion & Soret Coefficient, ESA): No report. [Background: Fluids and gases are never at rest. This statement is in apparent contradiction with our experience: when we pour water in a glass and wait until all flows have disappeared and the temperature of the liquid is in equilibrium with that of the room, we see that water appears to be completely at rest. However, if we were able to see the individual molecules of water with a very powerful microscope, we would discover that they are incessantly moving and collide with each other following frantic, random paths even if the liquid appears to be quiescent at naked eye. Scientists are interested in observing and measuring such movements because they reveal important, practical information: how fast does heat propagates in a fluid? How fast do liquid mixtures mix? Such phenomena occur in absence of a macroscopic flow, that is when the fluid appears to be at rest, and are called heat and mass diffusion respectively. While the theoretical prediction of heat and mass diffusion is still quite challenging, its measurement is a standard laboratory practice, but may become extremely difficult or impossible when dealing with mixtures of many liquids, due to the fact that such measurement needs to be carried out when the fluid is quiescent, a condition sometimes impossible to achieve on ground. This is precisely the objective of the SODI DSC experiment carried out on board the International Space Station: the measurement of diffusion in mixtures of liquids. By using very sensitive optical techniques, it will be possible to measure mass diffusion, compare with current theories, and improve our present understanding of how molecules move in liquid mixtures. The results will be used by the large team of scientists involved in the project to try to understand which of the many existing theories for mass diffusion is correctly predicting the experimental behavior.]
SOLAR (Solar Monitoring Observatory, ESA): The Sun Visibility Window #56 ended on 8/29. Measurements were performed with both instruments. Few minor Sun sensor glitches and Analog Input Board (AIB) failure events were encountered, with no impact on the planned scientific program. SolACES is now put back in heated mode in preparation of the HTV3 unberthing on 9/6.
SOLO (Sodium Loading in Microgravity): No report.
Space-DRUMS (Space Dynamically Responding Ultrasonic Matrix System): No report.
Space Food (JAXA): No report.
SPHERES (Synchronized Position Hold, Engage, Reorient, Experimental Satellite): No report.
SPHINX (SPaceflight of Huvec: an Integrated eXperiment, ESA): No report.
SPICE (Smoke Point In Co-flow Experiment): No report.
SPINAL (Spinal Elongation): No report.
SPRINT: "Aki, great job with your Sprint VO2max this week! The PI has received the data and is in the process of reviewing it. Thank you for your diligence!"
SS-HDTV (Super Sensitivity High Definition Camera, JAXA): Mission completed last week.
STP-H3 (Space Test Program - Houston 3): The STP-H3 data packet loss problem was corrected on 8/24 after the update to the timeliner sequence that accounts for both STP-H3 and SCAN payload packets. MHTEX is currently priming the Capillary Pumped Loop (CPL) in preparation for additional testing. VADER continues to characterize the performance of the Aerogel blanket attached to the backside of the experiment. Canary downloaded files from the reboost event last week and is analyzing data taken for previous events. DISC took new images this week and continues to process images that were taken in previous weeks.
SWAB (Characterization of Microorganisms & Allergens in Spacecraft): No report.
TASTE IN SPACE (ESA): No report.
THERMOLAB (ESA): "Dear Suni, the THERMOLAB science team confirmed the validity of your first session performed 10 days ago (on 8/7)."
TRAC (Test of Reaction & Adaptation Capabilities): Planned.
TREADMILL KINEMATICS: "Thanks, Suni, for your 2nd Treadmill Kinematics session! Thanks, Joe, for your 5th Treadmill Kinematics session, and thanks in particular for the calibration at the end."
TRIPLELUX-B (ESA): No report.
UMS (Urine Monitoring System (NASA): No report.
VASCULAR (CSA): "We received the VASCULAR Podcast -thanks, Joe, we appreciate this. It will be useful for our outreach program."
VCAM (Vehicle Cabin Atmosphere Module, NASA): No report.
VESSEL ID System (ESA): Nominal data acquisition with the NorAIS receiver, with a couple of small permanent losses - 3 distinct events between 8/28 and 8/29. [Background: As the ISS circles Earth, it has been tracking individual ships crossing the seas beneath. An investigation hosted by ESA in COL module has been testing the viability of monitoring global maritime traffic from the station's orbit hundreds of kilometers above since June 2010. The ship-detection system being tested is based on the AIS (Automatic Identification System), the marine equivalent of the air traffic control system. Astronauts were instrumental in enabling the COLAIS experiment, which is an in-orbit demonstration project of ESA's General Support Technology Program. COL was not originally outfitted with VHF antennas to capture the AIS signals; they were installed on the outside of the module during a spacewalk in November 2009, with the remaining piece of hardware, the ERNOBox control computer, installed inside COL along with the NORAIS receiver in May 2010.- The two operational phases with the first receiver from Norway, or NORAIS, which is operated by FFI/Norway, have been extremely successful, with data telemetry received by the N-USOC, in Trondheim, Norway, via ESA's COL-CC in Germany. Data has been received by NORAIS in almost continuous operation, and all modes of operation have worked extremely well. On a good day, approximately 400,000 ship position reports are received from more than 22,000 different ship identification numbers (Maritime Mobile Service Identity, or MMSI).-- The NORAIS Receiver has a sample mode that can collect the raw signal, digitize it and send it to ground for analysis of signal quality, which is proving very helpful in making additional improvements/ refinements to the system. This is used both to investigate the signal environment and to evaluate the performance of new receiver technologies on the ground. Several hundred data sets have been collected and processed with new candidate algorithms for next generation receivers.-- From the assessment of these data sets, an updated version of the decoder algorithm has been worked. The development benefits from the investigations of the sampled data and ongoing work in other ESA projects. The firmware was uploaded to the NORAIS Receiver through the station's communications network. This upgrade #1 ("NORAIS Receiver FPGA firmware v18"), was activated on 1/20/2012.-- The on-orbit data of the NORAIS Receiver v18 have been analyzed since and show very good results. The teams are confident in the operation and performance of v18 and have now preliminary results of the comparison of the performance of the upgraded NORAIS Receiver (v18) relative to the version operated prior to the upgrade (v16).-- Changes of the signal environment on ISS can influence the number of correctly decoded messages, which makes it important to compare the results of this upgrade to a period running the old algorithm with a similar background level.-- The daily averages are calculated for 11 days for both receiver versions. For the upgrade, the period considered for comparison is 1/21-1/31/2012, which are the first 11 days of operation. When selecting the period for the reference data it was important to find a period with the same background signal level as the 11 days with the upgraded NORAIS Receiver. The period from 11/27 - 12/7/2011 was. Even though the two 11 day periods are 45 days apart, the ship traffic should not be very different around the world, except for some regions in the north that may be hampered by sea ice.-- The performance has been studied as the average number of decoded messages per day for the current upgrade v18 of the firmware and the original NORAIS Receiver software. The improvement is the ratio of these numbers (so average numbers of messages per day before the upgrade divided by number of messages after the upgrade). The number of messages from ships in various geographic areas shows a variation in the ratio of messages from 1.2 to 2.0, whereas the ratio of MMSI's ranges from 1.1 to 1.9. The improvement in the Mediterranean is almost a factor of 2.0 in number of messages, and more than 1.6 in number of distinct ships per day. The improvement in other high-traffic zones, at the Gulf of Mexico and East Asia, is even higher.]
VESSEL IMAGING (ESA): No report. [Background: It is known that the ability of blood vessels to vasoconstrict - the ability of the muscular vessel wall to narrow the diameter of the blood vessel - is impaired during and after a human has been in space. "Vessel Imaging" is using the Ultrasound scanner on board the ISS to take images of the five different blood vessels in the lower abdomen and in the legs to study what changes occur to cause the blood vessels to be less able to vasoconstrict. For each vessel, a 5 second scan is performed to observe the blood vessel during several heart beats, followed by a scan where the ultrasound scan-head is tilted to allow a "cut through the blood vessel wall". The same scans are also performed before flight, and these pre-flight images are used as the baseline to which the in-flight data is compared with. The images are analyzed to detect any changes in the blood vessel wall properties, such as wall thickness, elasticity or structure, changes in the size of the blood vessel or blood flow (volume) while the crewmember is in orbit.]
VIABLE (eValuatIon And monitoring of microBiofiLms insidE the ISS Payload Touch, NASA): Suni Williams completed the touch activity and also took pictures of the VIABLE bags. Analysis of these pictures is part of the science return for VIABLE.
VO2max (NASA): No report.
VLE (Video Lessons ESA): No report.
WAICO #1/#2 (Waving and Coiling of Arabidopsis Roots at Different g-levels; ESA): No report.
YEAST B (ESA): No report.
YOUTUBE SpaceLab: No report.
CEO (Crew Earth Observation): Through 8/26 the ground has received 8,105 of ISS CEO frames from Expedition 32 for review and cataloging. "We are pleased to report that we have received imagery with times corresponding to our CEO target request times as follows: Yellow River Delta, China - 51 frames - target acquired - seasonal requirements met for this target - target can be REMOVED from our active request list; Baku, Azerbaijan - 33 frames - target not acquired due to clouds; Ljubljana, Slovenia - 51 frames - target acquired - under review for requirements; Lagoon of Venice, Italy - target acquired - seasonal requirements met for this target - target can be REMOVED from our active request list; Budapest, Hungary - 46 frames - target not acquired; Kinshasa-Brazzaville - 41 frames in 2 sessions - under evaluation for content; Tropical Storm Isaac - 8 frames - target acquired - under evaluation for content; Krasnodar Floods, southern Russia - 17 frames - target acquired - under evaluation for requirements; Belgrade, Serbia - 19 frames - under review for content; Cordillera Blanca Glaciers, Peru - 40 frames - under evaluation for content; and Bern, Switzerland - 9 frames - under evaluation for content. Your recent, well-composed view of a strand plain in coastal Peru was published on the NASA/GSFC Earth Observatory website this past weekend. Your image nicely illustrates this special coastal feature and the relationship of wave action, coastal currents, and river sediment discharge in the building of successive beach lines; in this case the process is possibly linked to El Nino events. Nice going, crew!"
CEO targets uplinked for today were Yamoussoukro, Cote d'Ivoire (CAPITAL CITIES COLLECTION: Nadir pass over this capital city of about a quarter of a million. Shooting a near-nadir strip to acquire this target. The large reservoir Lake Kossou is the best visual cue), Moscow, Russia (CAPITAL CITIES COLLECTION: Looking well left for this capital city of 11.5 million people. Visual cue is a major forest boundary trending northeast towards the city), Falmouth, England (HMS BEAGLE SITE: Near nadir pass over Falmouth, a port city in southwestern England. Charles Darwin ended his famous voyage of discovery here in 1836. Falmouth is located on a prominent, narrow inlet on the south coast of Cornwall. Overlapping mapping frames of the urban and surrounding rural areas were requested), Remnants of Tropical Storm Isaac, US Midwest (INTERNATIONAL DISASTER CHARTER (IDC): Tropical Storm Isaac has drenched portions of Louisiana with more than 25 inches of rain. The area has just been designated an activation area by the IDC. Looking right of track, where breaks in the clouds permit, for areas of flooding. Flooded areas will show up particularly well in sun glint), and Slate Islands Impact, Ontario, Canada (IMPACT CRATER SITE: Looking right. The Slate Islands are the tight cluster of islands just off the north shore of Lake Superior. The islands mark the center of a 30 km-diameter impact structure formed ~450 million years ago. ISS had two passes: the uplinked pass had better illumination).
Significant Events Ahead (all dates Eastern Time and subject to change):
09/04/12 -- U.S. EVA-19 (planned)
09/06/12 -- HTV3 undocking
09/08/12 -- HTV3 reentry
09/16/12 -- Soyuz TMA-04M/30S undock/landing - 5:56pm/9:20pm
(End of Increment 32)
09/25/12 -- ATV3 undocking
10/15/12 -- Soyuz TMA-06M/32S launch - K.Ford (CDR-34)/O.Novitsky/E.Tarelkin
10/17/12 -- Soyuz TMA-06M/32S docking
11/01/12 -- Progress M-17M/49P launch
11/03/12 -- Progress M-17M/49P docking
11/12/12 -- Soyuz TMA-05M/31S undock/landing (End of Increment 33)
12/05/12 -- Soyuz TMA-07M/33S launch - C.Hadfield (CDR-35)/T.Mashburn/R.Romanenko
12/07/12 -- Soyuz TMA-07M/33S docking
12/25/12 -- Progress M-16M/48P undocking
12/26/12 -- Progress M-18M/50P launch
12/28/12 -- Progress M-18M/50P docking
03/19/13 -- Soyuz TMA-06M/32S undock/landing (End of Increment 34)
04/02/13 -- Soyuz TMA-08M/34S launch - P.Vinogradov (CDR-36)/C.Cassidy/A.Misurkin
04/04/13 -- Soyuz TMA-08M/34S docking
05/16/13 -- Soyuz TMA-07M/33S undock/landing (End of Increment 35)
05/29/13 -- Soyuz TMA-09M/35S launch - M.Suraev (CDR-37)/K.Nyberg/L.Parmitano
05/31/13 -- Soyuz TMA-09M/35S docking
09/xx/13 -- Soyuz TMA-08M/34S undock/landing (End of Increment 36)
09/xx/13 -- Soyuz TMA-10M/36S launch - M.Hopkins/TBD (CDR-38)/TBD
09/xx/13 -- Soyuz TMA-10M/36S docking
11/xx/13 -- Soyuz TMA-09M/35S undock/landing (End of Increment 37)
11/xx/13 -- Soyuz TMA-11M/37S launch - K.Wakata (CDR-39)/R.Mastracchio/TBD
11/xx/13 -- Soyuz TMA-11M/37S docking
03/xx/14 -- Soyuz TMA-10M/36S undock/landing (End of Increment 38)
// end //