Table 1.
Magnetic connectivity between spacecraft and the Sun.
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) | (10) |
|---|---|---|---|---|---|---|---|---|---|
| PFSS (a) |
ADAPT-WSA (a) |
||||||||
| Spacecraft | r | Long. (b) | Lat. (b) | Vobs | Long. (b) | Lat. (b) | Polarity | Long. (b)(c) | Lat. (b)(c) |
| (au) | (°) | (°) | (km s−1) | (°) | (°) | (O, M) | (°) | (°) | |
| Flare | – | 203 | −17 | – | – | – | – | – | – |
| BepiColombo | 0.63 | 180.3 | −0.2 | 400 (d) | 202.5 | 62.4 | (+, +) | 204.1 ± 2.8 | 62.2 ± 2.1 |
| PSP | 0.42 | 104.3 | 3.8 | 328 | 146.7 | 28.6 | (+, +) | 131.1 ± 8.4 | 65.3 ± 1.1 |
| Solar orbiter | 0.84 | 215.8 | 0.4 | 375 | 266.7 | −21.5 | (–, –) | 267.9 ± 0.2 | −21.8 ± 0.1 |
| STA | 0.97 | 260.5 | −7.2 | 385 | 329.1 | −32.7 | (–, –) | 329.3 ± 0.3 | −32.5 ± 0.2 |
| L1 | 1.00 | 314.2 | −5.4 | 601 | 347.4 | −21.8 | (–, –) | 347.4 ± 0.1 | −22.5 ± 0.1 |
Notes. Columns (1)–(4) present the respective observer and its location in Carrington coordinates (with the first row providing the flare location). Column (5) lists the measured solar wind speed. Columns (6)–(7) and (9)–(10) provide the backmapped magnetic footpoints of the observer at the solar surface using the simple PFSS and the ADAPT-WSA models, respectively. Column (8) presents the magnetic field polarity observed (O) in situ and modeled (M) by ADAPT-WSA and PFSS.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.