Transmission Time From Dscovr To Earth

Solar Wind Propagation and GOES Solar Data

Transmission Time from DSCOVR to Earth

With the current speed of the solar wind, it takes approximately 60 minutes for the solar wind to propagate from the Deep Space Climate Observatory (DSCOVR) to Earth. This transmission time is important for providing real-time information about solar activity and its potential impact on Earth's geomagnetic environment.

GOES Solar X-ray Data

The plot on this page displays the most recent 24-hour solar X-ray data from the primary GOES satellite. This data provides valuable insights into the intensity and frequency of solar flares, which can significantly impact Earth's atmosphere and ionosphere.

Solar Activity Indicators

In addition to the solar X-ray data, this page also monitors other indicators of solar activity, including: * Solar flares: Sudden bursts of energy released by the Sun that can disrupt Earth's radio communications and power grids. * Sunspot regions: Darker areas on the Sun's surface that indicate regions of intense magnetic activity. * Coronal holes: Openings in the Sun's plasma atmosphere that allow the solar wind to escape into space. * Solar Cycle: The 11-year cycle of solar activity, from solar minimum to solar maximum. * Real-time magnetometer data: Measurements of the Earth's magnetic field, indicating the presence and strength of solar storms.

Radiation Storm Forecast

This page also provides a 3-day forecast of radiation storms, which are caused by coronal mass ejections. These forecasts help scientists and policymakers prepare for potential disruptions to satellite communications, power systems, and human health.