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Heliospheric Weather Expert Service Centre - Statistical Products |
This section provides information on the solar wind density at Earth during a particular solar rotation. The solar wind parameters can be used to identify the periods which drive enhanced geomagnetic activity.
The analysis is based on the OMNI database of upstream solar wind parameters produced by NASA.
A particular solar rotation can be selected from the pull down menu. The time interval display cannot be edited directly. A range can be specified that is used to identify intervals where the solar wind density is within those limits. Horizontal red lines may be shown on the plot indicating the time intervals that match the user criteria. Vertical dotted lines may be displayed indicating where the current time would map assuming recurrence of the solar wind density between solar rotations.
The mouse can be used to zoom the time selection (the Y scale is fixed). To zoom out extend the zoom range beyond the full plot range. A zoom range fully before(left)/after(right) of the plotted time interval will select a range of the same duration before/after the current plot. Pressing submit will recalculate the display for the new interval.
This web page forms part of the European Space Agency's network of space weather services and service development activities, and is supported under ESA contract number 4000134036/21/D/MRP. For further product related information or enquiries contact the helpdesk. E-mail: helpdesk.swe@esa.int All publications and presentations using data obtained from this site should acknowledge RAL Space and The ESA Space Safety Programme. For further information about space weather in the ESA Space Safety Programme see: https://www.esa.int/spaceweather Access the ESA SWE Portal here: https://swe.ssa.esa.int.