Solar Wind
solar_windFetch real-time DSCOVR L1 solar wind data—Bz, speed, and proton density—to monitor southward IMF for geomagnetic storm risk.
Instructions
Get real-time DSCOVR L1 solar wind data.
Shows interplanetary magnetic field (Bz component), solar wind speed, and proton density from the DSCOVR satellite at L1 (~1.5M km sunward). Southward Bz (negative) drives geomagnetic storms.
Input Schema
| Name | Required | Description | Default |
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No arguments | |||
Output Schema
| Name | Required | Description | Default |
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No arguments | |||