Woolrich Women Fw s Fw Tundracat Coconut/Red Snow Boot Boot Coconut/Red Hunting Plaid b7d99b5




Leather
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Rubber sole
Shaft measures approximately 8\" from arch
Waterproof leather and fleece upper
Fully wooly analog insulated lining, -25 comfort rating
 
Solar wind
speed: 419.2 km/sec
density: 2.9 protons/cm3
more data: ACE, DSCOVR
Updated: Today at 0551 UT X-ray Solar Flares
6-hr max: A4
0424 UT Jul09
24-hr: A4
0424 UT Jul09
explanation | more data
Updated: Today at: 0500 UT Daily Sun: 09 July 18 The sun is blank-- no sunspots. Credit: SDO/HMI

Sunspot number: 0
What is the sunspot number?
Updated 09 Jul 2018

Spotless Days
Current Stretch: 12 days
2018 total: 99 days (52%)

Woolrich Women Fw s Fw Tundracat Coconut/Red Snow Boot Boot Coconut/Red Hunting Plaid b7d99b5 - starnow.website

2017 total: 104 days (28%)
2016 total: 32 days (9%)
Woolrich Women Fw s Fw Tundracat Coconut/Red Snow Boot Boot Coconut/Red Hunting Plaid b7d99b5 2015 total: 0 days (0%)
2014 total: 1 day (<1%)
2013 total: 0 days (0%)
2012 total: 0 days (0%)
2011 total: 2 days (<1%)
2010 total: 51 days (14%)
2009 total: 260 days (71%)

Updated 09 Jul 2018


The Radio Sun
10.7 cm flux: 72 sfu
explanation | more data
Updated 09 Jul 2018

Current Auroral Oval:
Switch to: Europe, USA, New Zealand, Antarctica
Credit: NOAA/Ovation Planetary K-index
Now: Kp= 1 quiet
24-hr max: Kp= 1
quiet
explanation | more data
Interplanetary Mag. Field
Btotal: 3.3 nT
Bz: 0.2 nT north
more data: ACE, DSCOVR
Updated: Today at 0551 UT Coronal Holes: 09 Jul 18
Solar wind flowing from this minor coronal hole could reach Earth on or about July 13th. Credit: SDO/AIA
Noctilucent Clouds The season for noctilucent clouds in he northern hemisphere is underway. Check here daily for the latest images from NASA's AIM spacecraft.
Switch view: Europe, USA, Asia, Polar Updated at: 07-08-2018 14:55:03 SPACE WEATHER
NOAA Forecasts
Woolrich Women Fw s Fw Tundracat Coconut/Red Snow Boot Boot Coconut/Red Hunting Plaid b7d99b5 Updated at: 2018 Jul 08 2200 UTC
FLARE
0-24 hr
24-48 hr
CLASS M
01 %
01 %
CLASS X
01 %
01 %
Geomagnetic Storms:
Probabilities for significant disturbances in Earth's magnetic field are given for three activity levels: active, minor storm, severe storm Updated at: 2018 Jul 08 2200 UTC Mid-latitudes
0-24 hr
24-48 hr
ACTIVE
30 %
15 %
MINOR
05 %
05 %
SEVERE
01 %
01 %
High latitudes
0-24 hr
24-48 hr
ACTIVE
15 %
15 %
MINOR
30 %
25 %
SEVERE
35 %
20 %
 
Monday, Jul. 9, 2018
What's up in space          

All-inclusive Northern Lights trips in Tromsø, Norway. Small groups, big experiences! Highly qualified guides ensure unique and unforgettable adventures with a personal touch. Visit Explore the Arctic

 

MARS VISIBLE IN BROAD DAYLIGHT: Astronomers have long known that the brightest planets can be seen with the naked eye in daylight. Usually this means Venus and Jupiter. Now Mars has joined the club. On July 6th in Trieste, Italy, Giorgio Rizzarelli saw the Red Planet with his unaided eye--a pinprick of dusty orange piercing the morning blue even after sunrise. He took these pictures, which simulate the view without optics. Browse: Mars Photo Gallery.

WHITE SUNSPOT: This weekend, observers of the sun have been waiting for something to emerge over the sun's eastern limb. We knew it was there because of a farside solar flare on July 6th. Today it arrived, and it appears to be a white sunspot:

The correct name of this phenomenon is "faculae." It is a cousin of sunspots.

Regular dark sunspots are magnetic islands on the surface of the sun. Magnetic fields in these areas are thousands of times stronger than Earth's magnetic field. Sunspot magnetic fields are so strong, they block the flow of heat from the nuclear furnace below. They appear dark because they are relatively cool compared to their surroundings.

Faculae are also made of magnetic fields. However, the magnetism of faculae is concentrated in much smaller bundles than in sunspots. Instead of blocking heat from below, they essentially form corridors that allow us to see into sun's hot interior, creating an apparent bright spot on the surface of the sun.

It is still possible that a dark core will follow these faculae over the limb in the hours ahead, establishing the region as a normal sunspot group. Stay tuned. Free: Solar Flare Alerts

Realtime Space Weather Photo Gallery

ONE RING ABOVE HOBBITON: Two weeks ago, the students of Earth to Sky Calculus traveled to New Zealand for an unprecedented launch of space weather balloons over Earth's 8th continent. To help fund their trip, they sent this ring of power to the stratosphere:

You can have it for $129.95. On the southern winter solstice, June 21st, the ring flew 109,580 feet above New Zealand's north island, passing almost directly above Hobbiton, the movie set for the Lord of the Rings. The band is made of golden-colored tungsten and inscribed with the authentic Mordor script of the One Ring. Along with the ring, you'll receive a greeting card showing the item in flight and telling the story of its journey to the edge of space.

Far Out Gifts: Earth to Sky Store
All proceeds support hands-on STEM education

WHY ARE NOCTILUCENT CLOUDS BLUE? Observers of noctilucent clouds (NLCs) often describe their color as "electric blue." This high-voltage photo taken July 7th by Pentti Arpalahti of Helsinki, Finland, is a great example:

But why? What makes these clouds of frosted meteor smoke the color of an electric discharge? It turns out, electricity has nothing to do with it.

NLCs are blue for two reasons: (1) The clouds consist of tiny ice crystals about the size of particles in cigarette smoke. Cigarette smoke looks blue, too, and for the same reason. Tiny particles scatter blue light better than other colors. (2) Ozone! Research in the 1970s revealed that some of the sunlight hitting noctilucent clouds first passes through Earth's ozone layer. Ozone tends to scatter red light, while allowing blue to pass. Sunbeams hitting noctilucent clouds have thus been pre-conditioned for blue.

Realtime Noctilucent Cloud Photo Gallery


Realtime Aurora Photo Gallery


  All Sky Fireball Network Every night, a network of NASA all-sky cameras scans the skies above the United States for meteoritic fireballs. Automated software maintained by NASA's Meteoroid Environment Office calculates their orbits, velocity, penetration depth in Earth's atmosphere and many other characteristics. Daily results are presented here on Spaceweather.com.

On Jul. 8, 2018, the network reported 16 fireballs.
(15 sporadics, 1 July Pegasid)

In this diagram of the inner solar system, all of the fireball orbits intersect at a single point--Earth. The orbits are color-coded by velocity, from slow (red) to fast (blue). [Larger image] [movies]

  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 July 9, 2018 there were 1912 potentially hazardous asteroids.
Recent & Upcoming Earth-asteroid encounters: Asteroid
Date(UT)
Miss Distance
Velocity (km/s)
Diameter (m)
2018 NQ
2018-Jul-03
10.4 LD
24.5
132
2018 MB7
2018-Jul-04
2.8 LD
11.6
62
2018 NJ
2018-Jul-07
2.4 LD
6
10
2018 NM
2018-Jul-17
1.4 LD
6.7
19
2018 LQ2
2018-Aug-27
9.4 LD
1.5
41
2016 GK135
2018-Aug-28
16.8 LD
2.8
9
2016 NF23
2018-Aug-29
13.3 LD
9
93
1998 SD9
2018-Aug-29
4.2 LD
10.7
51
2018 DE1
2018-Aug-30
15.2 LD
6.5
28
2001 RQ17
2018-Sep-02
19.3 LD
8.3
118
2015 FP118
2018-Sep-03
12.3 LD
9.8
490
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.   Cosmic Rays in the Atmosphere

Readers, thank you for your patience while we continue to develop this new section of Spaceweather.com. We've been working to streamline our data reduction, allowing us to post results from balloon flights much more rapidly, and we have developed a new data product, shown here:

This plot displays radiation measurements not only in the stratosphere, but also at aviation altitudes. Dose rates are expessed as multiples of sea level. For instance, we see that boarding a plane that flies at 25,000 feet exposes passengers to dose rates ~10x higher than sea level. At 40,000 feet, the multiplier is closer to 50x. These measurements are made by our usual cosmic ray payload as it passes through aviation altitudes en route to the stratosphere over California.

What is this all about? Approximately once a week, Spaceweather.com and the students of Earth to Sky Calculus fly space weather balloons to the stratosphere over California. These balloons are equipped with radiation sensors that detect cosmic rays, a surprisingly "down to Earth" form of space weather. Cosmic rays can seed clouds, trigger lightning, and penetrate commercial airplanes. Furthermore, there are studies ( #1, #2, #3, #4) linking cosmic rays with cardiac arrhythmias and sudden cardiac death in the general population. Our latest measurements show that cosmic rays are intensifying, with an increase of more than 13% since 2015:


Why are cosmic rays intensifying? The main reason is the sun. Solar storm clouds such as coronal mass ejections (CMEs) sweep aside cosmic rays when they pass by Earth. During Solar Maximum, CMEs are abundant and cosmic rays are held at bay. Now, however, the solar cycle is swinging toward Solar Minimum, allowing cosmic rays to return. Another reason could be the weakening of Earth's magnetic field, which helps protect us from deep-space radiation.

The radiation sensors onboard our helium balloons detect X-rays and gamma-rays in the energy range 10 keV to 20 MeV. These energies span the range of medical X-ray machines and airport security scanners.

The data points in the graph above correspond to the peak of the Reneger-Pfotzer maximum, which lies about 67,000 feet above central California. When cosmic rays crash into Earth's atmosphere, they produce a spray of secondary particles that is most intense at the entrance to the stratosphere. Physicists Eric Reneger and Georg Pfotzer discovered the maximum using balloons in the 1930s and it is what we are measuring today.

  Essential web links NOAA Space Weather Prediction Center
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  The official U.S. government space weather bureau Atmospheric Optics   The first place to look for information about sundogs, pillars, rainbows and related phenomena. Solar Dynamics Observatory   Researchers call it a "Hubble for the sun." SDO is the most advanced solar observatory ever. STEREO   3D views of the sun from NASA's Solar and Terrestrial Relations Observatory Solar and Heliospheric Observatory   Realtime and archival images of the Sun from SOHO. Daily Sunspot Summaries   from the NOAA Space Environment Center NOAA 27-Day Space Weather Forecasts   fun to read, but should be taken with a grain of salt! Forecasts looking ahead more than a few days are often wrong. Aurora 30 min forecast   from the NOAA Space Environment Center Heliophysics   the underlying science of space weather Spaceweather.com welcomes two supporters of science communication: SEO Phoenix AZ and CRAS, the Conservatory of Recording Arts and Sciences. Only the best social media jobs in the United States     Look no further to find the best Comox Valley Real Estate listings and homes for sale     Okanagan Real Estate     Buy real active Instagram followers Guide for best car parts at prettymotors.com     Chicago SEO Expert     Search Kelowna Real Estate Listings & Homes for Sale easily.
Find help on all Calgary Homes For Sale and Real Estate Listings. Great source for Edmonton Real Estate Listings & Homes For Sale     Reviews here can help you to pick up best memory foam mattresses.   These links help Spaceweather.com stay online. Thank you to our supporters!   more links...
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