A s t r o A l e r t 14 May 2005 Solar Terrestrial Dispatch www.spacew.com MAJOR SOLAR FLARE PROMPTS AN AURORA WARNING The Sun is known for producing energetic spurts of activity, even during the less active periods around the solar sunspot minimum years. We are now a little more than one year from reaching the solar minimum. The frequency of energetic solar events has diminished over the last year, as has the number of sunspots that pepper the face of the Sun. But as has been the case with most solar cycles in recorded history, the Sun is not always quiet. It occasionally hiccups and produces large and complex sunspots capable of influencing space weather at the Earth. We are currently experiencing one of those 'hiccups.' Several large sunspots have appeared recently that have had the potential to produce energetic solar flare activity. Region 10759, now nearing the central solar meridian, spawned a major class M8.0 solar x-ray flare at 16:57 UTC on 13 May. The event was associated with strong radio bursts across the spectrum. Such bursts have the potential to disrupt cellular phone services when the Sun is aligned with the direction of cellular signal propagation (most dominantly near sunrise and sunset when solar elevation angles are more in-line with cellular signal trajectories). This event has also been blamed for producing a weak space radiation storm, where energetic particles (protons) arrive from the Sun travelling at near relativistic velocities. Such storms have the potential to affect the health and stability of satellites orbiting the Earth. Perhaps most significantly, this solar flare was associated with a coronal mass ejection that appears to be directed squarely at the Earth. Sometime on 15 May (perhaps during the early to mid UTC hours of 15 May, corresponding to the late evening to early morning hours of 14/15 May for North Americans), this cloud of solar plasma will impact the Earth's magnetosphere and energize it. What follows will depend upon the energy of the impact and the orientation of the imbedded solar magnetic fields that interact with the Earth's magnetic field. If the imbedded magnetic fields are oriented appropriately, they will generate a potentially strong geomagnetic storm and produce auroral activity ("northern lights") that may become visible across extensive middle latitude regions (central United States through perhaps central Europe, New Zealand and southern Australia). Given our proximity to the solar minimum and the decreasing frequency of auroral storm events, it may be prudent to watch the skies carefully for activity this weekend (particularly on Saturday and Sunday nights). Current information can be found at www.spacew.com or www.sec.noaa.gov. Those who succeed in observing activity are encouraged to report their observations to the Global Auroral Activity Observation Network at: www.spacew.com/submitsighting.html. A near-realtime accounting of reported sightings can be found at: www.spacew.com/www/auroras.html. This disturbance is expected to last roughly 18 to 24 hours and may only provide an opportunity to observe auroral activity for one evening. There may be additional opportunities to observe activity over the coming week, as the active sunspot complex responsible for producing this disturbance may yet spawn additional major flares and Earthward-directed CME's in the days ahead. A copy of the official Middle Latitude Auroral Activity Warning is appended below for your convenience. MIDDLE LATITUDE AURORAL ACTIVITY WARNING Issued: 05:05 UTC on 14 May 2005 Solar Terrestrial Dispatch www.spacew.com VALID BEGINNING AT: 00:00 UTC 15 MAY 2005 VALID UNTIL: 23:00 UTC (6 pm EST) ON 16 MAY HIGH RISK PERIOD: 15 MAY (UTC DAYS) MODERATE RISK PERIOD: 15-16 MAY PREDICTED ACTIVITY INDICES: 14, 70, 30, 12 (14 - 17 MAY) POTENTIAL MAGNITUDE OF MIDDLE LATITUDE AURORAL ACTIVITY: MODERATE TO HIGH POTENTIAL DURATION OF THIS ACTIVITY: MAIN BELT = 12-18 HOURS MINOR BELT = 18-24 HOURS ESTIMATED OPTIMUM OBSERVING CONDITIONS: NEAR OR PRIOR TO LOCAL MIDNIGHT EXPECTED LUNAR INTERFERENCE: LOW OVERALL OPPORTUNITY FOR OBSERVATIONS FROM MIDDLE LATITUDES: GOOD AURORAL ACTIVITY *MAY* BE OBSERVED APPROXIMATELY NORTH OF A LINE FROM... (THIS LINE IS VALID *ONLY* IF FAVORABLE STORM CONDITIONS OCCUR) OREGON TO SOUTHERN IDAHO AND NORTHERN UTAH TO WYOMING TO NEBRASKA TO NORTHERN MISSOURI TO SOUTHERN ILLINOIS TO KENTUCKY TO VIRGINIA. ACTIVITY *MAY* ALSO BE OBSERVED APPROXIMATELY NORTH OF A LINE FROM... (THIS LINE IS VALID *ONLY* IF FAVORABLE STORM CONDITIONS OCCUR) CENTRAL FRANCE TO NORTHERN SWITZERLAND TO SOUTHERN GERMANY TO THE CZECH REPUBLIC TO POLAND TO CENTRAL RUSSIA. NEW ZELAND AND SOUTHEASTERN AUSTRALIA SHOULD ALSO BE ABLE TO SPOT PERIODS OF ACTIVITY IF SUITABLE STORM CONDITIONS MATERIALIZE DURING DARKNESS. SYNOPSIS... A major class M8.0 solar flare on 13 May has been associated with a coronal mass ejection that appears to be strongly Earthward-directed. A major geomagnetic and auroral storm is expected to materialize on 15 May when the CME impacts the Earth. Periods of moderate to strong auroral storm conditions could be observed with this disturbance. Many middle latitude observations of activity should be possible after the disturbance arrives. Impact is expected sometime during the early to mid UTC hours of 15 May and the disturbance should persist well into 16 May. For North American observers, the first opportunity to observe activity may come as early as the very early morning hours (pre-dawn) of 15 May. The next (slightly less favorable) opportunity will be on the evening of 15 May, although depending on when the disturbance arrives, storm conditions may be on the decline by the time darkness falls over North America. Observers are encouraged to watch for activity. As we approach the solar minimum, these opportunities to observe the "northern lights" will diminish in frequency. This disturbance may have the potential to produce fairly vigorous auroral storming for brief periods of time. This warning will remain valid through 24:00 UTC (6 pm EDT) on 16 May. It will be updated or allowed to expire at that time. For updated information, visit: http://www.spacew.com/aurora/forum.html. For real-time plots of current activity, visit: http://www.spacew.com/plots.html PLEASE REPORT VALID OBSERVATIONS OF AURORAL ACTIVITY TO: http://www.spacew.com/submitsighting.html --------------------------------- Yahoo! Mail Mobile Take Yahoo! Mail with you! Check email on your mobile phone.