49.003 UE Oriole 4 was launched from Andoya Space Center, Norway on November 30, 2015. The CAPER mission intended to establish the role and nature of Alfvén wave acceleration in the cusp and discover the causes of the observed differences in the Langmuir waves in the cusp versus the nightside. CAPER also included the first ever wave-particle correlator measurements to be made in the cusp. The results affect a range of NASA programs in geospace, planetary, heliospheric and astrophysical sciences and are pertinent to multiple objectives of NASA’s Heliophysics research program.
36.293 UG Chakrabarti/University of Massachusetts Lowell - November 24, 2015 Planet Imaging Concept Testbed Using a Rocket Experiment (PICTURE)→
36.393 UT Black Brant 9 was launched from White Sands Missile Range, NM on November 25, 2015. The PICTURE mission was designed to observe the planetary environment around the star Epsilon Eridani and to directly image the planet.
36.310 GT Black Brant 9 was launched from Wallops Island, VA on October 7, 2015. This mission is a test flight of the new Black Brant Mk4 sustainer motor. The primary objective is to characterize the motor performance in a Black Brant IX configuration. The secondary objective of this mission is to provide NASA and NSROC an opportunity to test new technology experiments.
39.012 DR Bernhardt/Naval Research Laboratory - September 16, 2015
Charged Aerosol Release Experiment (CARE) II→
39.012 DR Black Brant XI was launched from Andoya Rocket Range, Norway on September 16, 2015.The CARE II mission examined the effect of artificially-created, charged-particulate layers on the scatter of UHF, L-Band and S-Band radars. The artificial particles were created from 37 CRV7 C14 motors ignited in the ionosphere. CARE II studied the exhaust plume physics including MHD waves and electric fields. The optical signature was measured from scattered sunlight and ion-molecule-electron reactions.
36.291 US Winebarger/University of Alabama - September 3, 2015
Chromospheric Lyman-Alpha Spectro Polarimeter (CLASP)→
36.291 US Terrier-Black Brant was launched from White Sands Missile Range, NM on September 3, 2015.The aim of CLASP mission was to achieve the first measurement of magnetic field in the upper chromosphere and transition region of the Sun through the detection and measurement of Hanle effect polarization of the Lyman alpha line.
36.282 US Kankelborg/Montana State University
- August 27, 2015
Multi-Order Solar EUV Spectrograph (MOSES)→
36.282 US Terrier-Black Brant was launched from White Sands Missile Range, NM on August 27, 2015. The purpose of the MOSES mission was to obtain line intensity images for Ciii 459.3A and Ne vii 465.2A at 1.2” resolution over a 20’ x 10’ field of view with reasonable cadence (approx.. 45 s) and obtain simultaneous line width and doppler shifts for the Ne vii line.. The cadence will be nominally lower than that of MOSES-1 due to the necessarily longer exposure times for Ne vii.
The RockSat-X student mission, 46.012 UO Koehler, was launched from Wallops Island, VA on Wednesday, August 12, 2015. RockSat-X carrier experiments developed by University students from around the country.
36.313 NP Black Brant IX was launched from Wallops Island, VA on July 7, 2015. The primary objective of this mission was to provide a technology test flight opportunity for researchers from NASA Ames Research Center and NASA Glenn Research Center.
41.113 UO Terrier-Improved Orion was launched from Wallops Island, VA on June 25, 2015. The primary objective of this effort is to conduct the RockOn Space Flight Workshop that is intended to provide University level students and instructors with a space flight opportunity that involves minimal cost, minimal time investment, minimal complexity, and minimal impact to the NASA Sounding Rockets Program.
36.300 UE Terrier-Black Brant was launched from White Sands Missile Range, NM on May 21, 2015. The primary objective for this mission is to provide an underflight calibration for the EUV Variability Experiment (EVE) aboard the NASA Solar Dynamics Observatory (SDO) satellite. The EVE program provides solar EUV irradiance data for NASA’s Living with the Star (LWS) program, including near real-time data products for use in operational atmospheric models that specify the space environment and to assist in forecasting space weather operations.
36.292 UH McEntaffer/University of Iowa - May 2, 2015
Off-plane Grating Rocket for Extended Source Spectroscopy (OGRESS)
36.292 UH Terrier-Black Brant was launched from White Sands Missile Range, NM on May 2, 2015. The OGRESS instruments provided high spectral resolving power for large diffuse X-ray sources. The science target was the Cygnus Loop supernova remnant which is one of the brightest and largest soft X-ray emitters in the sky. The observation provided global plasma conditions from this object which are typified by interactions between the supernova blast wave and a precursor formed cavity wall. The payload also contains a critical NASA X-ray technology ― off-plane reflection grating arrays. Combined with parallel technology development efforts, this mission will provide a flight proving platform for future X-ray missions.
46.008 UO Terrier-Improved Malemute was launched from Wallops Island, VA on April 18, 2015. This mission is an advanced student mission and a follow on to the RockOn and RockSat-C student payloads. The mission provides experimenters from several schools the opportunity to fly a payload, of their design, exposed to the space environment. The design of a payload and vehicle with pre-defined mechanical, power, instrumentation and flight performance capabilities were developed to provide exposure to the environment for these university student experimenters. There were six experiments on this mission.
The RockSat-X mission is currently going through integration and testing activities at NASA Wallops Flight Facility.
36.292 UH McEntaffer/University of Iowa - March 13, 2015
Off-plane Grating Rocket for Extended Source Spectroscopy (OGRESS) →
The OGRESS mission is currently going through integration and testing activities at NASA Wallops Flight Facility.
36.299 DR Terrier-Black Brant was launched from White Sands Missile Range, NM on February 25, 2015. The Department of Defense’s Space Test Program, based at Kirtland Air Force Base sponsored this mission which carried a payload designed by scientists and engineers from the Air Force Research Laboratory’s (AFRL) Space Vehicles Directorate also at Kirtland Air Force Base. The launch vehicle which is designed to reach an altitude over 100 miles provided an opportunity for the payload to release small amounts of Samarium vapor to create clouds of plasma, or ionized gas into the near-vacuum of space to study processes responsible for formation of the Earth’s ionosphere. Dr. Todd Pedersen/AFRL is the Principal Investigator.
49.002 UE Oriole-4 was launched from Poker Flat Research Range, AK on January 28, 2015. The ASSP mission attempts to answer questions about what the contributions of small spatial scale and rapid temporal scale fluctuations of electric fields are relative to the larger-scale electrodynamic processes? ASSP investigated the small scale spatial and temporal variability in the E-field that is known to contribute significantly to the overall heating at high latitudes. and the statistics of small spatial and temporal scales relative to the much larger scale electric field patterns. Read More
46.009 & 46.010 UE Collins - January 26, 2015
Mesosphere-Lower Thermosphere Turbulence Experiment (M-TEX)→
46.009 and 46.010 UE Terrier-Improved Malemutes were launched from Poker Flat Research Range, AK on January 26, 2015. The M-TEX mission objectives include obtaining a better understanding of how meteorological processes control the impact of solar processes on the Earth’s atmosphere through investigating the atmosphere’s response to auroral, radiation belt, and solar energetic particles, and associated effects on nitric oxides and ozone.Read More
41.111 & 41.112 UE Larsen - January 26, 2015
Mesospheric Inversion-layer Stratified Turbulence experiment (MIST)→
41.111 and 41.112 UE Terrier-Improved Orions were launch launched from Poker Flat Research Range, AK on January 26, 2015.The purpose of the Mesospheric Inversion-layer Stratified Turbulence (MIST) mission is to look for evidence of changes in the stratified turbulence properties within long-lived mesospheric inversion layers in the atmosphere between 80km and 140km. Especially of interest is the structure function, i.e., power spectrum, of the turbulent fluctuations in that region. Read More
36.295 US Terrier-Black Brant was launched from White Sands Missile Range, NM on December 11, 2014. The FOXSI instruments test the fabrication and function of focusing optics for solar high energy x-ray observations in the 4-15 keV energy range. FOXSI observed the non-flaring “quiet” Sun and searched for non-thermal x-rays in these regions. These seven detectors are a pathfinder for future observatories investigating particle acceleration on the Sun. Read More
52.001 UE a Black Brant XII-A was launched from Andoya Rocket Range, Norway on November 24, 2014. The scientific objective of the mission is to identify mechanisms responsible for creating a region of enhanced neutral mass density at 400 km altitude that appears to be a permanent feature of Earth’s cusp-region thermosphere. Earth’s cusps are magnetic field features in the magnetosphere associated with regions through which plasma from the Sun can have direct access to the upper atmosphere. Neutral and ion flow fields in the region of the density anomaly will be measured to see if that flow is consistent with establishing the observed density enhancement. Read More
36.253 US Terrier-Black Brant was launched from White Sands Missile Range on November 6, 2014. The Rapid Acquisition Imaging Spectrograph Experiment (RAISE) has an extremely high speed scanning-slit imaging spectrograph designed to observe and analyze dynamics and heating of the solar chromosphere and corona on time scales as short as 100 ms, with TRACE-like spatial resolutions, and velocity sensitivity of 1-2 km/s. Read More.
The ASSP mission is currently going through integration and testing activities at NASA Wallops Flight Facility.
46.009 & 46.010 UE Collins - October 10, 2014 Mesosphere-Lower Thermosphere Turbulence Experiment (M-TEX)→
The M-TEX mission has completed most of the integration and testing activities at NASA Wallops Flight Facility.
The CAPER mission integration and testing activities at NASA Wallops Flight Facility.
36.288 DS VOURLIDAS/NRL - September 14, 2014
Very high Angular resolution Ultraviolet Telescope (VAULT 2.0)
The scientific observationsduring this mission included viewing the magnetic footprint-driven evolution and heating of the solar atmosphere. Coronal loops, special hot structures, and other features were present during the observation period with the sun being very active.Read More
36.308 GT Terrier-Black Brant was launched from Wallops Island, VA on August 28, 2014. The primary objective of this mission was to test an ejection system for a future science mission, as well as, test a new High Temperature Antenna. Read More
36.289 US DIDKOVSKY/UNIVERSITY OF SOUTHERN CALIFORNA July 22, 2014
Degradation Free Spectrometers (DFS)
36.289 US Terrier-Black Brant was launched from White Sands Missile Range on July 22, 2014. This was a re-fly of the 36.263 payload that contained the new prototype experiment instruments known as the Degradation Free Spectrometers (DFS) for Solar Physics. The mission objectives are to: Improve our knowledge of solar physics driven spectral variability over all solar cycle time scales through stable, radiometrically accurate spectral irradiance measurements in the highly dynamic EUV/soft X-ray range. These are improvements on the previous work for SDO/EVE/ESP and SOHO/SEM. Read More
46.007 GP Terrier-Improved Malemute was launched from Wallops Island, VA on July 2, 2014. The primary objective of this mission is to develop a new standard carrier for periodic technology demonstration missions. The secondary objective is to provide flight opportunity for several NSROC developmental systems and components. Read More
41.110 UO Terrier-Improved Orion was launched from Wallops Island, VA on June 26, 2014.The RockOn workshop is intended to be an introductory flight opportunity to provided exposure to, and spark interest in, space based science missions. This will be accomplished by flying two classes of experiments. First time participants will generally fly the simpler kit built experiment. As educational institutions gain more experience, it is expected they will progress towards developing their own unique RockSat-C class experiments. Read More
36.285 UG FRANCE/UNIVERSITY OF COLORADO - May 24, 2014
Colorado High-resolution Echelle Stellar Spectrograph (CHESS)
36.285 UG Black Brant IX was launched from White Sands Missile Range, NM on May 24, 2014. This mission, the Colorado High-resolution Echelle Stellar Spectrograph (CHESS), is designed to enable new scientific studies of the Local Interstellar Medium (LISM). The LISM provides an opportunity to study general ISM phenomena up close and in three dimensions, including interactions of different phases of the ISM, cloud collisions, cloud evolution, ionization structure, thermal balance, turbulent motions, etc. Understanding the structure of the LISM is important in evaluating the cosmic ray environment and the potential habitability of nearby exoplanets. Read More
36.235 US Black Brant IX was launched from White Sands Missile Range, NM on May 3, 2014. The scientific objective of the Hydrogen Polarimetric Explorer (HYPE) mission is to measure Hydrogen Lyman light reflected by interplanetary hydrogen (IPH) in the Geocorona. IPH is an important transitional medium that flows from its origin in the local interstellar cloud (LIC) through the LIC-solar wind boundary zones into the inner heliosphere, where it interacts with the solar wind, and radiation pressure. HYPE will measure the line shape of the IPH, yielding information about the thermal structure of the interplanetary medium, the shape and location of the LIC-solar wind boundary areas, and the ionization state of the ILC. Read More