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AsteriaStar
Live data · 8 providers · 23 products

Space Weather

The Sun is measured continuously, and the measurements are public. This is AsteriaStar's operational space-weather centre: real values from NOAA and NASA, each shown with the time it was taken and the file it came from.

Right now

Space weather now

Current conditions →
  • Solar wind

    Live

    470 km/s

    Moderate

    2026-09-17 08:07 UTC

  • Planetary Kp

    Recent

    1.67

    Quiet

    2026-09-17 03:00 UTC

  • Geomagnetic scale

    Live

    None

    no storm in the last 24 h

    2026-09-17 08:13 UTC

  • X-ray flux

    Live

    B2.1

    current GOES class

    2026-09-17 08:11 UTC

Source: NOAA Space Weather Prediction Center. Times are UTC, as published by the provider.

Full current conditions →

The section

  • Current conditions

    Everything being measured right now, in one view.

  • Solar wind

    Speed, density and the interplanetary magnetic field at L1.

  • Geomagnetic activity

    The planetary K-index, observed and forecast, and NOAA's alerts.

  • Solar activity

    Flares, active regions, radio flux and catalogued eruptions.

  • Aurora

    NOAA's OVATION forecast and how far the oval reaches.

  • Events

    Flares, CMEs, storms and particle events as catalogued by NASA.

What space weather is

The Sun does not simply shine. It sheds a supersonic plasma — the solar wind — that carries its magnetic field out past every planet, and it occasionally throws off far larger structures: flares that brighten the whole X-ray sky in minutes, and coronal mass ejections that launch billions of tonnes of magnetised plasma into interplanetary space. Space weather is what happens when that reaches Earth.

Earth's magnetic field deflects most of it. What gets through depends less on how fast the wind is blowing than on which way its embedded magnetic field points: when the interplanetary field turns southward, opposite to Earth's own field at the dayside boundary, the two can reconnect and energy pours into the magnetosphere. That is what drives aurora, and what disturbs power grids, satellite navigation and high-frequency radio.

The measurements on these pages come from spacecraft at the L1 Lagrange point, roughly 1.5 million kilometres sunward of Earth, from the GOES satellites in geostationary orbit, and from a worldwide network of ground magnetometers. L1 gives something like half an hour to an hour of warning, depending on how fast the wind is travelling — which is why the same page shows both an observation time and a modelled arrival time and never conflates them.

The scales

Solar flare classes

Flares are ranked by peak X-ray brightness in the 1–8 Ångström band, each class ten times stronger than the last.

A
Background level; negligible effects.
B
Minor; no noticeable effects.
C
Small flares with few noticeable consequences.
M
Medium flares; can cause brief radio blackouts and minor radiation storms.
X
The most intense flares; can trigger planet-wide radio blackouts and strong radiation storms.

Geomagnetic storm scale (G1–G5)

NOAA's operational scale for geomagnetic disturbance, keyed to the planetary K-index.

G1
Minor: weak power-grid fluctuations; aurora at high latitudes.
G2
Moderate: aurora reaches mid-high latitudes.
G3
Strong: aurora at mid-latitudes; possible satellite and navigation effects.
G4
Severe: widespread aurora and grid/navigation impacts.
G5
Extreme: aurora far from the poles; major infrastructure risk.

The planetary K-index

A quasi-logarithmic index of geomagnetic disturbance over each three-hour interval, averaged across a global network of magnetometer stations.

Kp 0
Very quiet; aurora confined to high polar latitudes.
Kp 3
Unsettled; aurora possible at high latitudes.
Kp 5
Minor geomagnetic storm (G1); aurora may reach mid-high latitudes.
Kp 7
Strong storm (G3); aurora may be seen at mid-latitudes.
Kp 9
Extreme storm (G5); aurora possible far from the poles.

Where the data comes from

  • NOAA Space Weather Prediction Center

    NOAA / National Weather Service

    Public domain (US Government work). No licence fee and no redistribution restriction.

    No key requirement and no published rate limit: SWPC serves these products as static JSON files. AsteriaStar polls no faster than each product's own publication cadence and caches every response, so a page view is not a provider request.

    Provider documentation →

  • NASA DONKI

    NASA Goddard Space Flight Center / Community Coordinated Modeling Center

    Public domain (US Government work), subject to NASA's media usage guidelines.

    The CCMC web service documents no rate limit and requires no key. (The same catalogue is mirrored behind api.nasa.gov, which does require a key and limits it to 1,000 requests an hour; AsteriaStar uses the documented key-less CCMC service instead.) Responses are cached for fifteen minutes, so each event feed costs at most four requests an hour.

    CCMC states that “the real-time space weather information and simulations stored in DONKI should be considered only as prototyping quality and in research context”. DONKI events are shown here as a curated research catalogue, not as an operational alert service — that role belongs to SWPC.

    Provider documentation →

  • JPL Solar System Dynamics / CNEOS

    NASA Jet Propulsion Laboratory, California Institute of Technology

    Public domain (US Government work), NASA/JPL-Caltech.

    JPL publishes a Fair Use Policy rather than a numeric limit: requests must be “reasonably necessary”, automated processes must not be “unnecessarily frequent, repetitive, or redundant”, only ONE request may be open at a time, and processes must back off on errors. AsteriaStar serialises JPL requests and stops asking after three consecutive failures — within a server instance, which is the honest scope: this deployment is serverless, so a second instance has its own queue and its own failure count. What bounds the rate across instances is the response cache in front of these pages, which is measured in hours: a page view is not a provider request, and the products are re-fetched when a cached page revalidates, not when someone reads it.

    JPL states of Sentry impact probabilities: “The probability computation is complex and depends on a number of assumptions that are difficult to verify. For these reasons the stated probability can easily be inaccurate by a factor of a few, and occasionally by a factor of ten or more.” It also notes there is no guarantee any particular API remains available.

    Provider documentation →

  • NASA ISS Trajectory Data

    NASA Johnson Space Center, Flight Operations Directorate (TOPO)

    Public domain (US Government work), NASA/JSC.

    A static file on NASA's public-data store, regenerated every few days. No key, no documented rate limit. AsteriaStar fetches it at most once every six hours, which is far less often than it changes.

    This is the operational trajectory the station's flight controllers use, not a two-line element set: state vectors every four minutes in the mean equator and equinox of J2000, spanning fifteen days. It ENDS. Beyond the published span there is no trajectory, and the station manoeuvres — so a position past the end of the file would be a guess, and none is offered.

    Provider documentation →

  • IAU Minor Planet Center

    International Astronomical Union / Center for Astrophysics, Harvard & Smithsonian

    Public data of the IAU Minor Planet Center.

    The MPC publishes machine-readable data files rather than an API, with no registration, no credentials and no documented rate limit. AsteriaStar reads one of them — the NEO Confirmation Page, about six kilobytes — and caches it for ten minutes.

    The NEO Confirmation Page lists CANDIDATES, not discoveries. An entry may turn out to be an already-known object, a main-belt asteroid rather than a near-Earth one, or an artefact; most entries leave the page within days. The score is the MPC's estimate of how likely the object is a NEO, not a probability that it exists.

    Provider documentation →

  • NASA Eclipse Web Site

    NASA Goddard Space Flight Center

    Public domain (US Government work), and NASA states that permission to reproduce the data is granted WHEN ACCOMPANIED BY an acknowledgment — “Eclipse Predictions by Fred Espenak (NASA’s GSFC)” for the solar catalogue and “Eclipse Predictions by Fred Espenak and Jean Meeus (NASA’s GSFC)” for the lunar one. The right acknowledgment travels with every eclipse AsteriaStar shows.

    Static catalogue pages with no key, no registration and no documented rate limit. The two century tables AsteriaStar reads are about two hundred kilobytes together and are cached for a week, because the contents were computed once and do not change.

    Instants are Terrestrial Dynamical Time, and the ΔT needed to convert them to UTC is itself a prediction for future dates — accurate to a second or two for the coming decades, and progressively less so further out. The catalogue gives the circumstances of greatest eclipse; it is not a local-circumstances calculator, and AsteriaStar does not turn it into one.

    Provider documentation →

  • Launch Library 2

    The Space Devs

    Free public access as stated by the provider; attribution given on every surface that uses it.

    The provider states the database is free for up to 15 requests an hour without a key. AsteriaStar caches each response for thirty minutes and backs off for a quarter of an hour after three consecutive failures, so a rate-limit response is never answered with more requests. That cache is process-local and does not survive a cold start, so it is a BEST-EFFORT bound rather than a guaranteed two an hour: several serverless instances answering at once each pay their own first request. Keeping inside the provider's allowance therefore rests on the cache plus the CDN in front of it, not on a shared budget — there is no durable one.

    NOT an agency schedule. It is a community-maintained aggregation of announcements made by operators and agencies, and the operators change their own dates constantly. Every entry carries the provider's own confirmation timestamp and its own statement of how precisely the date is known, and both are shown — a launch scheduled to the quarter is not displayed as though it were scheduled to the second.

    Provider documentation →

  • MET Norway Weather API

    Norwegian Meteorological Institute (Meteorologisk institutt)

    NLOD 2.0 and CC BY 4.0. Attribution required; commercial use permitted.

    The provider requires an identifying User-Agent for server requests and asks browsers to identify themselves by the Origin header they send automatically, and states that anything over 20 requests a second per application needs a prior agreement. AsteriaStar makes ONE request per reader who explicitly asks for a forecast, from their own browser, and none at all otherwise — so the platform generates no baseline traffic at all.

    A general meteorological forecast. `cloud_area_fraction` is total cloud cover and is NOT astronomical seeing, sky transparency, or sky brightness — those are different quantities produced by different models, and a clear forecast with terrible seeing is an ordinary night. Only cloud cover is read, and it is never renamed.

    Provider documentation →

Every product, its cache window and this server's own request record are on the live provider health page. The same data is available through the public API.

Every value on these pages is fetched from NOAA SWPC or NASA CCMC and carries the provider's own timestamp. Nothing is simulated, interpolated or filled in: when a provider cannot be reached, the panel says so and shows no number. There is no overall “space weather score” here — the agencies publish scales, and a single figure invented on top of them would be an opinion wearing NOAA's authority.

Sources & references

The primary and reference sources this topic draws on.

  • NOAA SWPCNOAA Space Weather Prediction Center

    Space-weather forecasts and alerts: aurora (OVATION), the Kp index, and the G1–G5 geomagnetic storm scale.

  • NASA DONKINASA Community Coordinated Modeling Center

    The Space Weather Database Of Notifications, Knowledge, Information: solar flares, CMEs, and geomagnetic storms.

  • NASANational Aeronautics and Space Administration

    Mission data, planetary science, space telescopes, and public-domain imagery.

    Most NASA-produced imagery is in the public domain; individual items are checked for usage terms before publication.