SOLAR WEATHER
and some interesting space stuff

2010

compiled by Dee Finney

APRIL - 2010

PAGE 4

updated  -   4-30-10

 

THIS COMPILATION IS BEING DONE IN HONOR OF KENT STEADMAN
OF  www.cyberspaceorbit.com  who left his earthly abode in 2008

 

2008 SOLAR WEATHER

 

2009 SOLAR WEATHER
JANUARY - FEBRUARY - MARCH - APRIL - MAY  - JUNE - JULY -
AUGUST - SEPTEMBER - OCTOBER - NOVEMBER - DECEMBER

 

2010 SOLAR WEATHER

JANUARY - FEBRUARY - MARCH - APRILMAY - JUNE - JULY
AUGUST - SEPTEMBER - OCTOBER - NOVEMBER - DECEMBER

 

On January 17, there were 1092 potentially hazardous asteroids.
On February 17, there were 1100 potentially hazardous asteroids.
NOTE:  These are not 'new' asteroids'  merely newly discovered by people and their new telescopes.
On March 24, there were 1110 potentially hazardous asteroids.
On April 5, there are 1110 potentially hazardous asteroids.
On April 14, there are 1117 potentially hazardous asteroids.


On February 21, 2010 there were 1103 potentially hazardous asteroids.
Feb. 2010 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2009 UN3
Feb. 9
14.3 LD
12
1.2 km
2010 CK19
Feb. 17
0.9 LD
17
11 m
2001 FD58
Feb. 19
58.5 LD
17
0.9 km
2010 CJ18
Feb. 19
3.3 LD
18
20 m
2002 EZ11
Feb. 24
77.5 LD
18
1.0 km
Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach

Near-Earth Asteroids
Potentially Hazardous Asteroids (PHAs) are space rocks larger than approximately 100m that can come closer to Earth than 0.05 AU. None of the known PHAs is on a collision course with our planet, although astronomers are finding new ones all the time.

On March 5, 2010 there were 1110
 potentially hazardous asteroids.

March 2010 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2001 PT9
March 3
11.1 LD
15
305 m
4486 Mithra
March 12
73.5 LD
15
3.3 km
2001 FM129
March 13
44.1 LD
16
1.5 km
2010 FU9
March 18
1.5 LD
17
19 m
2010 EF43
March 18
5.0 LD
19
23 m
2010 FT
March 27
5.5 LD
20
33 m
2002 TE66
March 28
48.0 LD
15
940 m
Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach.

On April 14, there were 1117
potentially hazardous asteroids
April 2010 Earth-asteroid encounters:
Asteroid
Date(UT)
Miss Distance
Mag.
Size
2010 GV23
April 5
2.1 LD
19
12 m
2010 GF7
April 8
2.8 LD
18
30 m
2010 GA6
April 9
1.1 LD
16
27 m
2010 GM23
April 13
3.4 LD
17
47 m
2005 YU55
April 19
5.9 LD
15
185 m
2009 UY19
April 23
8.8 LD
18
87 m
2002 JR100
April 29
8.0 LD
19
65 m
Notes: LD means "Lunar Distance." 1 LD = 384,401 km, the distance between Earth and the Moon. 1 LD also equals 0.00256 AU. MAG is the visual magnitude of the asteroid on the date of closest approach.


 

 

 

 

 

TOWARD THE END OF TIME
IT'S THE DANGER OF THE SUN

THE RIDDLE OF THE STARS

NEW    A STAR NAMED HADES   NEW

Explore the Sunspot Cycle

 

phobos with lines

PHOBOS?

HOW DID ALL THOSE LINES GET THERE?

 

 

4-30-10
 

SUNSPOTS AHOY! Amateur astronomer Thomas Ashcraft of New Mexico reports a bipolar sunspot group forming in the sun's northeastern quadrant. He took these photos on April 30th around 1730 UT. Readers with solar telescopes are encouraged to monitor developments.



Current conditions
Solar wind
speed: 393.0 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: C1
1935 UT Apr30
24-hr: C1 1935 UT Apr30
explanation | more data
Updated: Today at: 2340 UT

Giant Blizzard Raging on Saturn Is Visible From Earth

Updated: 17 hours 38 minutes ago

SPACE.com Staff

Space.com
(April 30) - A massive blizzard is raging on Saturn - a storm so large and fierce NASA astronomers and amateur skywatchers can see it from Earth.

NASA's Cassini spacecraft currently orbiting Saturn has a front row seat to the otherworldly tempest and is recording the most detailed data yet of storms on the ringed planet. But amateur astronomers back on Earth have also managed to chip in on the Saturn blizzard stormwatch.

"We were so excited to get a heads-up from the amateurs," said Cassini scientist Gordon Bjoraker, a composite infrared spectrometer team member based at NASA's Goddard Space Flight Center in Greenbelt, Md.
saturn storm
Christopher Go, GSFC / JPL- Caltech / NASA
Amateur astronomer Christopher Go, who lives in the Philippines, took this image of the storm on Saturn at its peak on March 13. The arrow indicates the location of the storm.

The data showed a large, turbulent storm, dredging up a lot of material from the deep atmosphere and covering an area at least five times larger than the biggest blizzard that hit Earth so far this year - the "Snowmageddon" storm that blanketed the Washington, D.C. area in snow in February.

Saturn's 'storm alley'

Cassini's radio and plasma wave instrument and imaging cameras have been tracking thunder and lightning storms on Saturn for years in a region around Saturn's mid-latitudes that is nicknamed "storm alley."

But, gathering data on storms requires a tricky balancing act, since storms on Saturn can come and go on a time scale of weeks, while Cassini's imaging and spectrometer observations have to be locked in place months in advance.

Given these limitations, NASA sometimes enlists the help of amateur astronomers.

The radio and plasma wave instrument regularly picks up electrostatic discharges that are associated with the storms, so scientists have been sending periodic tips to amateurs, who can quickly go to their backyard telescopes and try to spy the bright convective storm clouds.

Amateur astronomers Anthony Wesley, Trevor Barry and Christopher Go received one of those notices in February, and were able to snap dozens of pictures over the next several weeks.

In fact, in late March, Wesley - who is based in Australia and was the first person spot the aftermath of an comet impact on Jupiter last summer - sent Cassini scientists an e-mail with a picture of the storm attached.

"I wanted to be sure that images like these were being seen by the Cassini team just in case this was something of interest to be imaged directly by Cassini or the Hubble Space Telescope," Wesley wrote.

Cassini scientists analyzed all the images in detail, including a picture from March 13 of the storm at its peak, taken by Go, who lives in the Philippines.

Saturn's storm season

Luckily, the composite infrared spectrometer happened to be targeting the latitude of the storms. The Cassini scientists had known there might be storms in that area, but were unsure when they might be active.

The Cassini spectrometer obtained data on March 25 and 26 that showed larger than expected amounts of phosphine, a gas typically found in Saturn's deep atmosphere, and an indicator that powerful currents were lifting material upward into the upper troposphere.

The spectrometer data also showed that the tropopause, which is the dividing line between the serene stratosphere and the lower churning troposphere, was about 1 degree Fahrenheit (minus 17.2 degrees Celsius) colder in the storm cell than in neighboring areas.

"A balloonist floating about 100 kilometers (62 miles) down from the bottom of Saturn's calm stratosphere would experience an ammonia-ice blizzard with the intensity of Snowmageddon," said Brigette Hesman, a composite infrared spectrometer team member and assistant research scientist at the University of Maryland.

"These blizzards appear to be powered by violent storms deeper down - perhaps another 100 to 200 kilometers (62 to 124 miles) down - where lightning has been observed and the clouds are made of water and ammonia," Hesman said.

The Cassini-Huygens mission is a joint project of NASA, the European Space Agency and the Italian Space Agency. The composite infrared spectrometer team is based at NASA's Goddard Space Flight Center in Greenbelt, Md.

* The Wildest Weather in the Galaxy
* The Rings and Moons of Saturn
* Top 10 Extreme Planet Facts
Filed under: Science
4-29-10 -  sunspot  1063- very small

sun - 4-29-10
WHAT IS COMING THIS WAY PAST THE SUN????  the devil in a speedboat???

Current conditions
Solar wind
speed: 366.4 km/sec
density: 3.9 protons/cm3
explanation | more data
Updated: Today at 0305 UT
X-ray Solar Flares
6-hr max: A7 2240 UT Apr29

24-hr: A7 1735 UT Apr29
explanation | more data
Updated: Today at: 2355 UT
4-28-10 - no su
nnspots

PLASMA RAIN: NASA's Solar Dynamics Observatory (SDO) has just observed a massive eruption on the sun. Movies ten times better than HDTV show billions of tons of material blasting into space while debris from the explosion rains around the blast site. Moon-sized fragments of plasma splash brightly when they land back on the sun's surface:

coronal rain
Above: "Plasma rain" photographed by SDO on April 19, 2010

Veteran solar physicists say they've never seen anything quite like it. The fluid detail of SDO's imagery is unprecedented, prompting NASA to dub it their "Hubble for the Sun."

SDO has already solved one mystery of plasma rain: The rain falls with puzzling slowness, seemingly resisting the sun's powerful gravity. What slows the descent? The phenomenon is explained in today's story from Science@NASA.



Current conditions
Solar wind
speed: 317.5 km/sec
density: 1.5 protons/cm3
explanation | more data
Updated: Today at 1255 UT
X-ray Solar Flares
6-hr max: A4 0950 UT Apr28

24-hr: A4 0515 UT Apr28
explanation | more data
Updated: Today at: 1245 UT
4-27-10 No sunspots

CORONAL HOLE: A dark hole has formed in the sun's atmosphere. NASA's STEREO-B spacecraft photographed it just hours ago:

coronal hole 4-28-10

It's a "coronal hole," a vast region where solar magnetic fields have opened up and allowed some of the sun's atmosphere to escape. The runaway atmosphere is heading our way in the form of a solar wind stream. High-latitude sky watchers should be alert for auroras when it arrives on or about May 3rd.


Current conditions
Solar wind
speed: 364.1 km/sec
density: 1.8 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A4
1825 UT Apr27
24-hr: A5
1400 UT Apr27
explanation | more data
Updated: Today at: 2340 UT
4-26-10 - No sunspots

POISED TO ERUPT: Already this month, the sun has produced two of the biggest eruptions in years. They occurred on April 13th and April 19th when magnetic filaments became unstable and exploded. Could it happen again today? A prominence on the eastern limb of the sun (photo) resembles the precursors of those two earlier blasts. Readers with solar telescopes are encouraged to monitor developments.

eruption of sun

Current conditions

Solar wind
speed: 349.7 km/sec
density: 9.0 protons/cm3
explanation | more data
Updated: Today at 1426 UT
X-ray Solar Flares
6-hr max: A8 0930 UT Apr26
24-hr: A8 0930 UT Apr26
explanation | more data
Updated: Today at: 1420 UT

 

4-25-10 - No sunspots

non-sunspot 4-25-10
non-sunspot 4-25-10
non-sunspot 4-25-10

According to RHESSi, it is in decay. it is not formed well. But I would consider it a spot myself. It looks to have magnetic loops. Looks like a coronal hole right in front of it too.

Dear RHESSI Collaborators,

Solar activity remains at very low levels. The target region continues to decay as it approaches the central meridian. No increase in activity expected at this time.

Current conditions
Solar wind
speed: 395.5 km/sec
density: 1.0 protons/cm3
explanation | more data
Updated: Today at 0130 UT
X-ray Solar Flares
6-hr max: B1 2300 UT Apr24
24-hr: B1 2300 UT Apr24
explanation | more data
Updated: Today at: 2355 UT
4-24-10 - No sunspots

Current conditions
Solar wind
speed: 327.6 km/sec
density: 0.1 protons/cm3
explanation | more data
Updated: Today at 2342 UT
X-ray Solar Flares
6-hr max: B1 2300 UT Apr24
24-hr: B1 2300 UT Apr24
explanation | more data
Updated: Today at: 2340 UT
4-23-10 - No sunspots

30 march prominence
A full-disk multiwavelength extreme ultraviolet image of the sun taken by SDO on March 30, 2010. False colors trace different gas temperatures. Reds are relatively cool (~60,000 K); blues and greens are hotter (> 1,000,000 K). [full-resolution image]
Credit: SDO/AIA


Current conditions
Solar wind
speed: 445.4 km/sec
density: 1.5 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: A4 2325 UT Apr23
24-hr: A4 2325 UT Apr23
explanation | more data
Updated: Today at: 2340 UT
4-22-10 - No sunspots

Current conditions
Solar wind
speed: 420.6 km/sec
density: 1.3 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A4 1905 UT Apr22
24-hr: A4 1730 UT Apr22
explanation | more data
Updated: Today at: 2340 UT
4-21-10 - No sunspots

STUNNING IMAGES OF THE SUN: NASA's Solar Dynamics Observatory is beaming back stunning new images of the sun, revealing our own star as never seen before. Even veteran solar physicists say they are amazed by the data. Click on the prominence, below, to see what everyone is so excited about:

30 March prominence
Must-see movies and images!

Related links:


Current conditions
Solar wind
speed: 438.8 km/sec
density: 0.6 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A3 2310 UT Apr21
24-hr: A3 1135 UT Apr21
explanation | more data
Updated: Today at: 2340 UT
4-20-10 - No sunspots

solar flare  4-20-10

A solar prominence erupts on April 19th at 1919 UT

The eruption catapulted a billion-ton CME out of the sun's atmosphere. SOHO saw that, too: movie. The expanding cloud is not heading for Earth, so we should feel no effects. The event was photogenic but not geoeffective

Current conditions
Solar wind
speed: 363.5 km/sec
density: 1.2 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A3 1950 UT Apr20
24-hr: A4 1215 UT Apr20
explanation | more data
Updated: Today at: 2340 UT
4-19-10 - No sunspots

Current conditions
Solar wind
speed: 346.8 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: A4 2140 UT Apr19
24-hr: A4 0005 UT Apr19
explanation | more data
Updated: Today at: 2340 UT
4-18-10 - No sunspots
Current conditions
Solar wind
speed: 380.1 km/sec
density: 0.3 protons/cm3
explanation | more data
Updated: Today at 2346 UT
X-ray Solar Flares
6-hr max: A5 1935 UT Apr18
24-hr: B1 0205 UT Apr18
explanation | more data
Updated: Today at: 2340 UT
4-17-10 - No sunspots

Current conditions
Solar wind
speed: 385.0 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A6 2330 UT Apr17
24-hr: B2 0555 UT Apr17
explanation | more data
Updated: Today at: 2340 UT
4-16-10 - no sunspots

Current conditions
Solar wind
speed: 463.6 km/sec
density: 2.2 protons/cm3
explanation | more data
Updated: Today at 1227 UT
X-ray Solar Flares
6-hr max: A4 0950 UT Apr16
24-hr: A4 0950 UT Apr16
explanation | more data
Updated: Today at: 1220 UT
4-15-10-  no sunspots

Current conditions
Solar wind
speed: 485.4 km/sec
density: 3.2 protons/cm3
explanation | more data
Updated: Today at 0053 UT
X-ray Solar Flares
6-hr max: A3 2025 UT Apr14
24-hr: A3 2025 UT Apr14
explanation | more data
Updated: Today at: 2355 UT

MIDWESTERN FIREBALL:  A brilliant fireball streaked across the USA on the evening of April 14th, startling observers in Minnesota, Iowa, Missouri and surrounding states.  Experts say it was a small asteroid, about a meter wide, that exploded in mid-air with an energy equivalent to some 20 tons of TNT.  National Weather Service radars detected the fireball's debris trail, resulting in maps that could help guide meteorite hunters to fragments on the ground. 

My own son, who was driving to work saw the ball of green light for about 5 seconds before it went behind some buildings and trees and out of sight in Milwaukee, WI.

Last night, around 10:05 pm CDT, sky watchers in Minnesota, Wisconsin, Iowa, Illinois and Missouri witnessed a brilliant green fireball streaking across the sky. Images from a rooftop webcam in Madison, Wisconsin, show a brilliant midair explosion:

asteroid 4-14-10
Credit: University of Wisconsin - AOS/SSEC

The fireball was caused by a small asteroid hitting Earth's atmosphere at a shallow angle. Preliminary infrasound measurements place the energy of the blast at 20 tons of TNT (0.02 kton), with considerable uncertainty. Bill Cooke of NASA's Meteoroid Environment Office estimates that the space rock was about 1 meter wide and massed some 1260 kg. "Fireballs of this size are surprisingly common," he notes. "They hit Earth about 14 times a month, on average, although most go unnoticed because they appear during the day or over unpopulated areas."

meteor over milwaukee wi

photo taken over Milwaukee, Wi - facing northeast
photo by John Wilke

Many readers have asked if fragments of the meteoroid might have reached Earth. The answer is "yes." Cooke advises looking directly underneath the fireball's debris trail, which was pinged by National Weather Service radars in Iowa. Click here and here for maps.

News video: from WISN in Milwaukee, Wisconsin; from a sheriff's dashcam in Elma, Iowa;

Not a gamma Virginid: Contrary to some reports, this fireball was not a member of the gamma Virginid meteor shower, a minor shower that peaks in mid-April. The fireball's timing and trajectory do not match what would be expected for a gamma Virginid.

Other people suggested it was part of a failed space shot by Russia the day before, or part of debris from a space war going on overhead.  There were planety of conspiracy theories going on as well.

VOLCANIC SUNSETS:  A cloud of ash from Iceland's Eyjafjallajokull volcano is drifting across Europe this week and causing sunsets of surpassing beauty. Europeans are encouraged to look west at the end of the day.  Bonus: If you don't live in Europe, look west anyway. Venus, Mercury and the crescent Moon are beaming through the twilight for all to see. Images: #1, #2, #3, #4, #5, #6, #7, #8, #9, #10.


4-14-10 - sunspot 1062

Current conditions
Solar wind
speed: 474.2 km/sec
density: 3.6 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: A3 2025 UT Apr14
24-hr: A3 2025 UT Apr14
explanation | more data
Updated: Today at: 2340 UT

4-13-10 - sunspot 1062

OMG! HUGE PROMINENCE: One of the biggest prominences in years erupted from the sun's northwestern limb today. The massive plasma-filled structure rose up and burst during a ~2 hour period around 0900 UT. Mark Townley sends this freeze-frame from his backyard observatory in Brierley Hill, West Midlands, UK:

CME 4-13-10

CME 4-13-10

CME 4-13-10

The eruption hurled a bright coronal mass ejection (CME) into space: SOHO movie. The cloud is not heading toward Earth, at least not directly. A glancing blow from the outskirts of the CME is possible two to three days from now, but any impact is likely to be mild. The eruption was more photogenic than geoeffective.

more images: from Steve Wainwright of Gower, South Wales UK; from Patrick Bornet of Saint Martin sur Nohain, Nièvre, France; from Robert Arnold of Isle of Skye, Scotland; from Les Observateurs Associés au Pic du Midi, France; from Gianfranco Meregalli of Milano Italy


Current conditions
Solar wind
speed: 375.5 km/sec
density: 1.8 protons/cm3
explanation | more data
Updated: Today at 1856 UT
X-ray Solar Flares
6-hr max: A3 1640 UT Apr13
24-hr: B2 0445 UT Apr13
explanation | more data
Updated: Today at: 1855 UT
4-12-10 - A new sunspot is appearing in the southern hemishphere  it can't be seen yet

NEW SUNSPOT: A new sunspot (provisionally numbered AR1062) is rapidly emerging in the sun's southern hemisphere. Readers with solar telescopes, now is the time to watch sunspot genesis in action. Images: from Thomas Ashcraft of New Mexico;

GEOMAGNETIC STORM: A coronal mass ejection hit Earth's magnetic field at approximately 12:30 UT on April 11th. The impact sparked a G2-class geomagnetic storm with auroras over Scandinavia, Scotland, Canada and northern-tier US states such as Maine, Michigan and Wisconsin.

Current conditions
Solar wind
speed: 434.6 km/sec
density: 2.3 protons/cm3
explanation | more data
Updated: Today at 1854 UT
X-ray Solar Flares
6-hr max: A3 1505 UT Apr12
24-hr: A6 0105 UT Apr12
explanation | more data
Updated: Today at: 1855 UT

4-11-10 - sunspot 1061

Current conditions
Solar wind
speed: 419.0 km/sec
density: 9.7 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A6 2305 UT Apr11
24-hr: A6 2305 UT Apr11
explanation | more data
Updated: Today at: 2340 UT
4-10-10 - sunspot 1061

INCOMING CME: Decaying sunspot 1060 delivered a parting shot on April 8th. The active region's magnetic field erupted, sparking a B3-class solar flare and hurling a faint coronal mass ejection (CME) almost directly toward Earth. Geomagnetic disturbances are possible when the cloud arrives on April 11th or 12th.

April 4th marked the beginning of a major solar wind storm, which is only now subsiding. The four-day event brought auroras to the lava fields of Iceland, created a kaleidoscopic display of moving color over Antarctica, and lured onlookers in Siberia outdoors for a quick "aurora dance." Really. Browse the gallery for photos.

UPDATED: April Northern Lights Gallery
[previous Aprils: 2009, 2008, 2007, 2006, 2005, 2004, 2003, 2002]

SUNGRAZING COMET:  This morning, the sun had a comet for breakfast. The icy visitor from the outer solar system appeared with little warning on April 9th and plunged into the sun during the early hours of April 10th. One comet went in, none came out.  Visit http://spaceweather.com to see a death plunge movie from the Solar and Heliospheric Observatory. 

The comet was probably a member of the Kreutz sungrazer family. Named after a 19th century German astronomer who studied them in detail, Kreutz sungrazers are fragments from the breakup of a giant comet at least 2000 years ago. Several of these fragments pass by the sun and disintegrate every day. Most are too small to see but occasionally a big fragment like today's attracts attention.

This has been an active year for big, bright sungrazers. There was one on Jan. 4th, one on March 12th, and now one today. Normally we see no more than 3 or 4 bright ones in a whole year; now we're seeing them almost once a month. It could be a statistical fluctuation or, maybe, a swarm of Kreutz fragments is nearing perihelion (closest approach to the sun).


SOLAR WIND STORM: The first major solar wind storm of the new solar cycle has come to an end. The event, which stretched from April 4th to April 8th, ignited auroras over both poles and many points in between.  Highlights include Northern Lights over an active volcano in Iceland, green skies in Minnesota, and a kaleidoscopic display of Southern Lights over Antarctica.  Start browsing the updated aurora gallery here:

comet 4-10-10

 http://www.spaceweather.com/aurora/gallery_01apr10_page5.htm

Current conditions
Solar wind
speed: 455.4 km/sec

density: 0.4 protons/cm3
explanation | more data
Updated: Today at 0115 UT
X-ray Solar Flares
6-hr max: A9 2035 UT Apr09
24-hr: B3 0450 UT Apr09
explanation | more data
Updated: Today at: 2355 UT
4-9-10 - sunspot 1061

Current conditions
Solar wind
speed: 460.3 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: A9 2035 UT Apr09
24-hr: B3 0450 UT Apr09
explanation | more data
Updated: Today at: 2340 UT
4-8-10 -sunspots 1060 and 1061

Current conditions
Solar wind
speed: 604.1 km/sec
density: 0.2 protons/cm3
explanation | more data
Updated: Today at 0234 UT
X-ray Solar Flares
6-hr max: A6 2355 UT Apr07
24-hr: A6 2355 UT Apr07
explanation | more data
Updated: Today at: 2355 UT

GEOSTORMS, CONTINUED: High-latitude sky watchers should remain alert for auroras. NOAA forecasters estimate a 45% chance of geomagnetic activity and a 10% chance of severe geomagnetic storms during the next 24 hours. The source of this activity is a fast and gusty solar wind stream that has been blowing around Earth for two days. [UPDATED: gallery].

 

4-7-10 - sunspots 1060 and 1061

Current conditions
Solar wind
speed: 601.7 km/sec   Keep your eye on the speed of the solar wind
density: 0.4 protons/cm3
explanation | more data
Updated: Today at 0322 UT
X-ray Solar Flares
6-hr max: A5 1805 UT Apr06
24-hr: B1 0400 UT Apr06
explanation | more data
Updated: Today at: 2355 UT
4-6-10 sunspot 1060 and 1061

The most powerful geomagnetic storm since December 2006 struck the Earth on Monday. The most powerful geomagnetic storm since December 2006 struck the Earth on Monday. The solar storm prompted NOAA to issue a Space Weather Advisory on Monday ordering all personnel on the space shuttle and International Space Station to take cover in specially designed compartment shields.

 

Charged particles come in the form of galactic cosmic rays, gamma rays, solar flares, and CME's. The Kp Index measures from 1 (mild) to 9 (severe). Monday's hit measured 7.

 

 

 

On 3 April, the SOHO spacecraft spotted a cloud of charged particles called a coronal mass ejection (CME) shooting from the Sun at 500 kilometers per second. This velocity suggested the front would reach Earth in roughly three days.

 

 

Equation: Charged Particles => Magnetic Field Shift => Shifting Ocean and Jet Stream Currents => Extreme Weather and Human Disruption (mitch battros).

 

 

 

A sharp gust of solar wind hit Earth's magnetosphere on Monday, April 5th, at approximately 0800 UT and sparked the strongest geomagnetic storm of the year.

 

"It hit earlier and harder than forecast," says Doug Biesecker of the US National Oceanic and Atmospheric Administration's (NOAA) Space Weather Prediction Center in Boulder, Colorado.



Current conditions
Solar wind
speed: 554.4 km/sec
density: 0.6 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: A5 1805 UT Apr06
24-hr: B1 0400 UT Apr06
explanation | more data
Updated: Today at: 2340 UT
4-5-10 -sunspot 1060 just came around the corner -  1057 and 1059 disappeared overnight

GEOMAGNETIC STORM: A sharp gust of solar wind hit Earth's magnetosphere today, April 5th, at approximately 0800 UT and sparked the strongest geomagnetic storm of the year. The event registered 7 on the 0-to-9 Kindex scale of magnetic disturbances. Although the storm is subsiding now, it is not over; high-latitude sky watchers should remain alert for auroras.  Latest images may be found in the gallery: http://www.spaceweather.com/aurora/gallery_01apr10_page3.htm

Current conditions
Solar wind
speed: 647.3 km/sec
density: 0.7 protons/cm3
explanation | more data
Updated: Today at 2243 UT
X-ray Solar Flares
6-hr max: B1
1700 UT Apr05
24-hr: B1
1250 UT Apr05
explanation | more data
Updated: Today at: 2240 UT
4-4-10 - sunspots 1057 and 1059

Current conditions
Solar wind
speed: 489.5 km/sec
density: 0.5 protons/cm3
explanation | more data
Updated: Today at 2342 UT
X-ray Solar Flares
6-hr max: A9
2005 UT Apr04
24-hr: B1
0900 UT Apr04
explanation | more data
Updated: Today at: 2340 UT

4-3-10 - sunspots 1057 and 1059

Current conditions
Solar wind
speed: 515.2 km/sec
density: 0.4 protons/cm3
explanation | more data
Updated: Today at 2343 UT
X-ray Solar Flares
6-hr max: A9
1810 UT Apr03
24-hr: B7
0950 UT Apr03
explanation | more data
Updated: Today at: 2340 UT
4-2-10 - sunspots 1057 and 1059

Current conditions
Solar wind
speed: 511.9 km/sec
density: 1.1 protons/cm3
explanation | more data
Updated: Today at 2345 UT
X-ray Solar Flares
6-hr max: A7
2315 UT Apr02
24-hr: A7
2315 UT Apr02
explanation | more data
Updated: Today at: 2340 UT
4-1-10 - sunspots - 1057 and 1059

SOLAR PROMINENCE: Today, amateur astronomers around the world are monitoring a huge prominence rising over the sun's northeastern limb. It's so big, it won't fit in the space provided. 

solar prominence - 4-1-10

Eric Roel took the picture just hours ago from his backyard observatory in Valle de Bravo, Mexico. Since then, the view has changed. Magnetic fields underpinning this magnificent structure are in a state of fairly rapid motion, pulling the plasma to and fro, offering a different profile to every observer. The whole thing could become unstable and collapse. Readers with solar telescopes are encouraged to monitor developments.

more images: from Andy Devey of Barnsley, South Yorkshire, England; from Cai-Uso Wohler of Bispingen, Germany;

Current conditions

Solar wind
speed: 466.3 km/sec
density: 1.5 protons/cm3
explanation | more data
Updated: Today at 2344 UT
X-ray Solar Flares
6-hr max: A4
1830 UT Apr01
24-hr: A6
0900 UT Apr01
explanation | more data
Updated: Today at: 2340 UT


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