Ieri pomeriggio, approfittando di un po di calma familiare e soprattutto visto il bel tempo, ho provato a vedere queste famigerate macchie del ciclo 23.
Devo dire che nel rifrattorino che ho non le avevo mai viste e sono rimasto subito esterefatto: le macchie si stagliavano nitide sul fondo bianco della fotosfera!
Ho pensato subito di provare una ripresa ed ho ottenuto questo risultato che voglio condividere con voi
I dati della ripresa e dell'elaborazione sono riportati sull'immagine
Nello
Effettivamente si, quelle sono le ultime ed impreviste macchie del ciclo 23, quello dato per chiuso fino a pochi giorni fa.
Infatti c'è stata una strana ripresa (anche se già osservata in passato) del vecchio ciclo, il 23°, mentre il nuovo il 24° era appena iniziato.
Le macchie da te fotografare sono state una sorpresa ed un'eccezione, infatti avendo la polarità del vecchio ciclo sono inequivocabilmente gli ultimi colpi del vecchio ciclo, mentre quelle nuove dovrebbero avere, ed hanno, polarità opposta.
Old Solar Cycle Returns
March 28, 2008: Solar Cycle 23, how can we miss you if you won't go away?
Barely three months after forecasters announced the beginning of new Solar Cycle 24, old Solar Cycle 23 has returned. (Actually, it never left. Read on.)
"This week, three big sunspots appeared and they are all old cycle spots," says NASA solar physicist David Hathaway. "We know this because of their magnetic polarity." On March 28th the Solar and Heliospheric Observatory (SOHO) made this magnetic map of the sun:
It shows the north and south magnetic poles of the three sunspots. All are oriented according to the patterns of Solar Cycle 23. Cycle 24 spots would be reversed.
What's going on? Hathaway explains: "We have two solar cycles in progress at the same time. Solar Cycle 24 has begun (the first new-cycle spot appeared in January 2008), but Solar Cycle 23 has not ended."
Strange as it sounds, this is perfectly normal. Around the time of solar minimum--i.e., now--old-cycle spots and new-cycle spots frequently intermingle. Eventually Cycle 23 will fade to zero, giving way in full to Solar Cycle 24, but not yet.
Meanwhile, on March 25th, sunspot 989, the smallest of the three sunspots, unleashed an M2-class solar flare. Flares are measured on a "Richter scale" ranging from A-class (puny) to X-class (powerful). M-class flares are of medium intensity. This one hurled a coronal mass ejection or "CME" into space (movie), but the billion-ton cloud missed Earth.
While the CME was still plowing through the sun's atmosphere, amateur radio astronomer Thomas Ashcraft heard "a heaving sound" coming from the loudspeaker of his 21 MHz shortwave receiver in New Mexico: listen. It was a Type II solar radio burst generated by shock waves at the leading edge of the CME. A thousand miles away in Virginia, David Thomas recorded the same emissions on a chart recorder he connected to his 20 MHz ham rig: look. "What a pleasant surprise," says Thomas.
Above: Sunspot counts vs. year: 2008 is a low point in the solar cycle. Smoothed curves are predictions of future activity. [More]
We could get more of this kind of activity in the next 7 to 10 days. It will take about that long for the sunspots to cross the face of the sun. The sun's rotation is turning the spots toward Earth, which means the next CME, if there is one, might not miss. CME strikes do no physical harm to Earth but they can cause Northern Lights, satellite glitches and, in extreme cases, power outages.
The real significance of these spots is what they say about the solar cycle, says Hathaway. "Solar Cycle 24 has begun, but we won't be through solar minimum until the number of Cycle 24 spots rises above the declining number of Cycle 23 spots." Based on this latest spate of "old" activity, he thinks the next Solar Max probably won't arrive until 2012.
Science@NASA
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