Abstract
A new type of solar neutron detector (NEM) was launched by the space shuttle Endeavour on July 16th, 2009 and it began collecting data on August 25th, 2009 at the International Space Station (ISS). In this paper we introduce not only preliminary results obtained by the NEM-FIB detector but also a possible solar neutron detection in association with the M3.7 solar flare on March 7, 2011.
| Original language | English |
|---|---|
| Pages | 169-172 |
| Number of pages | 4 |
| DOIs | |
| Publication status | Published - 2011 Jan 1 |
| Externally published | Yes |
| Event | 32nd International Cosmic Ray Conference, ICRC 2011 - Beijing, China Duration: 2011 Aug 11 → 2011 Aug 18 |
Other
| Other | 32nd International Cosmic Ray Conference, ICRC 2011 |
|---|---|
| Country | China |
| City | Beijing |
| Period | 11/8/11 → 11/8/18 |
Keywords
- Flares
- Particle acceleration at the sun
- Solar neutrons
ASJC Scopus subject areas
- Nuclear and High Energy Physics
Fingerprint Dive into the research topics of 'Measurement of high-energy neutrons at ISS by SEDA-AP-FIB'. Together they form a unique fingerprint.
Cite this
Koga, K., Goka, T., Matsumoto, H., Obara, T., Okudaira, O., Muraki, Y., & Yamamoto, T. (2011). Measurement of high-energy neutrons at ISS by SEDA-AP-FIB. 169-172. Paper presented at 32nd International Cosmic Ray Conference, ICRC 2011, Beijing, China. https://doi.org/10.7529/ICRC2011/V10/0370