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Space Weather Prediction Center

National Oceanic and Atmospheric Administration

Saturday, September 18, 2021 03:34:33

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NOAA Scales mini

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Space Weather Conditions
24-Hour Observed Maximums
R
no data
S
no data
G
no data
Latest Observed
R
no data
S
no data
G
no data
R1-R2 --
R3-R5 --
S1 or greater --
G
no data
R1-R2 --
R3-R5 --
S1 or greater --
G
no data
R1-R2 --
R3-R5 --
S1 or greater --
G
no data
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R
no data
S
no data
G
no data
Current Space Weather Conditions
R1 (Minor) Radio Blackout Impacts
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HF Radio: Weak or minor degradation of HF radio communication on sunlit side, occasional loss of radio contact.
Navigation: Low-frequency navigation signals degraded for brief intervals.
More about the NOAA Space Weather Scales

WAM-IPE

Global Ionosphere

WAM-IPE Global Ionosphere

Neutral Atmosphere

WAM-IPE Neutral Atmosphere

The coupled Whole Atmosphere Model-Ionosphere Plasmasphere Electrodynamics (WAM-IPE) Forecast System (WFS) provides a specification of ionosphere and thermosphere conditions with forecasts two days in advance in response to solar, geomagnetic, and lower atmospheric forcing. Model outputs are used at the Space Weather Forecast Office (SWFO) at SWPC for issuing warnings and alerts related to aviation communication and Global Navigation Satellite System (GNSS) scintillations. The real-time neutral density fields will also be available for orbit prediction and space traffic management purposes.

The WAM is an extension of the Global Forecast System (GFS) with a spectral hydrostatic dynamical core utilizing an enthalpy thermodynamic variable to 150 vertical levels on a hybrid pressure-sigma grid, with a model top of approximately 3 x 10-7 Pa (typically 400-600km depending on levels of solar activity). Additional upper atmospheric physics and chemistry, including electrodynamics and plasma processes, are included.
The IPE model provides the plasma component of the atmosphere. It is a time-dependent, global 3D model of the ionosphere and plasmasphere from 90 km to approximately 10,000 km. The flux-tube solver is based on the Field Line Interhemispheric Plasma (FLIP) model and flux-tube structures are defined by the International Geomagnetic Reference Field (IGRF). Seamless perpendicular plasma transport pole-to-pole and self-consistent electrodynamics are included.

WAM fields of winds, temperature, and molecular and atomic atmospheric composition are coupled to IPE to enable the plasma to respond to changes driven by the neutral atmosphere. The coupling is based on time-dependent 3D re-gridding in the space weather mediator. The model ingests solar wind and geomagnetic inputs, provided both by direct observation and as forecast by SWFO. The WAM-IPE Forecast System (WFS) provides products out to two days using these drivers as initialized by the data assimilation (DA) system.

The WAM state is updated using 3DVar DA in the lowest 60km of the atmosphere using a modified version of the Gridpoint Statistical Interpolation (GSI) software. An Incremental Analysis Update (IAU) method is used to apply the increment across the assimilation window to prevent the damping of tidal waves from the DA process. This comprises the WAM-IPE Data Assimilation System (WDAS).

The top two panels show the latest global Total Electron Content (TEC) and Maximum Usable Frequency (MUF) as forecasted by the WAM-IPE. The bottom two panels show the anomaly in TEC and MUF taking the difference between the latest values and a 10-day running average at the same universal time. The forecast is updated with the latest real-time and forecast solar and geomagnetic drivers at 0, 6, 12 & 18 UT.

The top plot shows the neutral density at 400 km and the bottom left plot shows the thermospheric column O/N2 ratio. The anomaly of neutral density at 400 km is shown in the bottom right plot, which is the percentage difference between the latest values and a 10-day running average at the same universal time. The forecast is updated with the latest real-time and forecast solar and geomagnetic drivers at 0, 6, 12 & 18 UT.

The model output files for 48 hours can be accessed here.