ONE OF THE HEALTH RISKS ASTRONAUTS FACE IS HIGH EXPOSURE TO IONIZING RADIATION FROM COSMIC RAYS AND SOLAR PARTICLE EVENTS Solicitation ID/Procurement Identifier: 80NSSC20K1173 Ultimate Completion Date: Wed Jul 31 17:00:00 GMT 2024
GALACTIC COSMIC RAYS (GCR) AND SOLAR PARTICLE EVENTS (SPES) ARE A MAJOR SOURCE OF CARCINOGENIC RISK FOR ASTRONAUTS ON PROLONGED SPACE MISSIONS. LARGE UNCERTAINTIES EXIST IN THE EXACT ESTIMATION OF CAN... Solicitation ID/Procurement Identifier: 80NSSC20K0732 Ultimate Completion Date: Fri Dec 10 18:00:00 GMT 2021
SOLAR ENERGETIC PARTICLE (SEP) EVENTS REQUIRE ACCURATE AND EFFICIENT FORECASTING FOR A WIDE RANGE OF OPERATIONS. Solicitation ID/Procurement Identifier: 80NSSC21K1388 Ultimate Completion Date: Sat Aug 31 17:00:00 GMT 2024
IMPROVED FORECASTING RELIABILITY OF SOLAR ENERGETIC PARTICLE (SEP) EVENTS IS IMPORTANT FOR BETTER-INFORMED AND MORE TIMELY SPACEWEATHER- RELATED DECISIONS IN INDUSTRY AND GOVERNMENT AGENCIES. Solicitation ID/Procurement Identifier: 80NSSC20K0287 Ultimate Completion Date: Mon Jan 31 18:00:00 GMT 2022
IMPULSIVE ION ESCAPE AT THE SUN-HSPHR EXECUTIVE SUMMARY: THE PREVAILING ASSUMPTION IS THAT MOST OF THE IONS IN 3HE-RICH SOLAR ENERGETIC PARTICLE (SEP) EVENTS ARE ACCELERATED THROUGH MAGNETIC RECONNECT... Solicitation ID/Procurement Identifier: NNX16AL66G Ultimate Completion Date: Wed Nov 27 18:00:00 GMT 2019
SCIENCE GOALS AND OBJECTIVES THE MOST ENERGETIC ELECTRONS IN SOLAR ENERGETIC PARTICLE (SEP) EVENTS CAN EXTEND TO MORE THAN SEVERAL MEV. AT THE SUN, ELECTRON BEAMS AT THESE ENERGIES ARE USUALLY ASSOCIATED WITH HARD X-RAYS AND GYRO-SYNCHROTRON RADIATIO Solicitation ID/Procurement Identifier: 80NSSC18K1232 Ultimate Completion Date: Fri Jun 25 17:00:00 GMT 2021
SOLAR FLARES ARE DIRECTLY RESPONSIBLE FOR SOME ASPECTS OF SPACE WEATHER, AND CAN INDICATE OTHER IMPENDING PHENOMENA (CORONAL MASS EJECTIONS AND SOLAR ENERGETIC PARTICLE EVENTS). PREDICTING SOLAR FLARE... Solicitation ID/Procurement Identifier: 80NSSC22K0273 Ultimate Completion Date: Sun Dec 31 18:00:00 GMT 2023
