Energetic Particles, MSU-TASPD

This experiment was one of several provided by the Theoretical and Applied Space Physics Division of the Skobeltsyn Institute of Nuclear Physics of Moscow State University. The experiments flew on the Soviet Zond, Luna, Mars, Venera, Vega, and Phobos interplanetary/planetary missions and measured energetic (MeV) particles in the interplanetary medium. The earliest missions (Zond 1 and 3) measured protons above 30 MeV. Later missions measured lower energy protons and some also measured fluxes toward and away from the sun. Many further details are available at: ftp://nssdc.gsfc.nasa.gov/pub/spacecraft_data/russian_msu/common_info.txt Data from all these experiments, unknown to NSSDC before 1999, were prepared at MSU and provided to NSSDC in 1999 in common ASCII formats and organizations.

本实验系莫斯科国立大学斯科普列茨金核物理研究所理论与应用空间物理分部提供的多项实验之一。这些实验搭载于苏联的‘飞向太阳系’、‘月球’、‘火星’、‘金星’、‘维加’以及‘火卫一’等行星际/行星探测任务中，对星际介质中的高能（MeV）粒子进行了测量。最早的探测任务（‘飞向太阳系’1号和3号）测量了超过30 MeV的质子。后续的任务测量了能量较低的质子，其中一些任务还测量了太阳朝向和背离的通量。更多详细信息可查阅：ftp://nssdc.gsfc.nasa.gov/pub/spacecraft_data/russian_msu/common_info.txt。这些实验的数据，在1999年之前对NASA空间科学数据中心（NSSDC）而言尚属未知，均由莫斯科国立大学在1999年整理并以通用的ASCII格式提供给NSSDC。