TY - JOUR
T1 - Minimum requirements for a solar probe mission
AU - Axford, W. I.
AU - Ip, W. H.
AU - McKenzie, J. F.
PY - 1996
Y1 - 1996
N2 - A minimum approach is considered for a solar probe mission making use of a probe/bus combination. In order to achieve the fundamental information required for the final understanding of solar wind acceleration and coronal heating - within a low cost envelope, the scientific merits and technical feasibilities of a set of appropriate experiments are evaluated. The total instrument package could weigh ≲ 10 kg with a total power consumption of < 30 watts. In this mission concept a carrier will bring the solar probe to swing past Jupiter and then release it at a distance between 0.3 and 1 AU to minimize the thermal and mechanical constraints. Also, as in the case of planetary atmosphere probes, batteries could be used to facilitate the probe measurements during the solar encounter. By the same token, batteries and solar cells could power the bus itself without the requirement of a RTG. Such a modular approach with clean interfaces and well-defined responsibilities is also advantageous to international cooperation. Finally, it is important that in order to have a clear picture of the origin of the high speed solar wind, the solar probe must reach its perihelion near solar minimum.
AB - A minimum approach is considered for a solar probe mission making use of a probe/bus combination. In order to achieve the fundamental information required for the final understanding of solar wind acceleration and coronal heating - within a low cost envelope, the scientific merits and technical feasibilities of a set of appropriate experiments are evaluated. The total instrument package could weigh ≲ 10 kg with a total power consumption of < 30 watts. In this mission concept a carrier will bring the solar probe to swing past Jupiter and then release it at a distance between 0.3 and 1 AU to minimize the thermal and mechanical constraints. Also, as in the case of planetary atmosphere probes, batteries could be used to facilitate the probe measurements during the solar encounter. By the same token, batteries and solar cells could power the bus itself without the requirement of a RTG. Such a modular approach with clean interfaces and well-defined responsibilities is also advantageous to international cooperation. Finally, it is important that in order to have a clear picture of the origin of the high speed solar wind, the solar probe must reach its perihelion near solar minimum.
UR - http://www.scopus.com/inward/record.url?scp=0043038376&partnerID=8YFLogxK
U2 - 10.1016/0273-1177(95)00502-6
DO - 10.1016/0273-1177(95)00502-6
M3 - 期刊論文
AN - SCOPUS:0043038376
SN - 0273-1177
VL - 17
SP - 85
EP - 90
JO - Advances in Space Research
JF - Advances in Space Research
IS - 3
ER -