get_solar_wind
Retrieve real-time solar wind magnetic field and plasma data from DSCOVR/ACE at L1 to identify geomagnetic storm drivers.
Instructions
Real-time solar wind from DSCOVR/ACE at L1: magnetic field + plasma.
Returns mag (Bx/By/Bz/Bt in nT, GSM) and plasma (density cm^-3, speed
km/s, temperature K) series for the chosen window. Sustained southward Bz
(negative) plus elevated speed is the classic geomagnetic-storm driver.
Input Schema
| Name | Required | Description | Default |
|---|---|---|---|
| window | No | 1-day |
Output Schema
| Name | Required | Description | Default |
|---|---|---|---|
| window | Yes | ||
| mag | Yes | ||
| plasma | Yes |