Directly under the Arctic Circle! Marianne's Arctic Xpress in Tromsø offers fjord, whale and wildlife tours by day, aurora tours by night. Book Now and get a 10% discount on combo day and night adventures. | | | SPOTLESS SUN: Today, the sun is blank--no sunspots. This latest episode of spotlessness continues a year-long trend of falling sunspot numbers, heralding the approach of Solar Minimum. Weekend forecast: blank suns and no solar flares. Free: Space Weather Alerts NEW MAPS OF THE SOUTH ATLANTIC ANOMALY: Researchers have long known that one of the van Allen Radiation Belts dips down toward Earth over South America, creating a zone of high radiation called "The South Atlantic Anomaly" (SAA). Since its discovery in 1958, the SAA has been shape-shifting, growing larger and intensifying. A map published just last week in the American Geophysical Union's journal Space Weather Quarterly outlines the anomaly with new precision: When a spacecraft in low-Earth orbit passes through the anomaly, "the radiation causes faults in spacecraft electronics and can induce false instrument readings," explains Bob Schaefer of the Johns Hopkins University Applied Physics Lab, lead author of the paper reporting the results. "We actually used these spurious signals to map out the radiation environment at an altitude of 850 km." Specifically, they looked at pulses of noise in an ultraviolet photometer carried aboard many polar orbiting Defense Meteorological Satellite Program (DMSP) satellites. When high-energy protons in the SAA pass through these sensors, they produce spurious signals--or, in the case of this study, valuable data. By monitoring the rate of spurious UV pulses, the researchers were able to trace the outlines of the anomaly and monitor its evolution over a period of years. They found that the anomaly is slowly drifting north and west at rates of 0.16 deg/yr and 0.36 deg/yr, respectively. Currently, it is most intense over a broad region centered on Sao Paulo, Brazil, including much of Paraguay, Uruguay, and northern Argentina. They also detected a seasonal variation: On average, the SAA is most intense in February and again in September-October. In this plot, yearly average counts have been subtracted to reveal the double-peaked pattern: One maximum coincides with an equinox, but the other does not. The authors were not able to explain the origin of this unexpected pattern. The solar cycle matters, too, as the data revealed a yin-yang anti-correlation with sunspots. "During years of high solar activity, the radiation intensity is lower, while during solar quiet years the radiation intensity is higher," writes Schaefer. According to orthodox thinking, the SAA reaches down from space to within about 200 km of Earth's surface. Below that altitude, its effects should be mitigated by the shielding of Earth's atmosphere and geomagnetic field. To test this idea, Spaceweather.com and Earth to Sky Calculus have undertaken a program to map the SAA from below using weather balloons equipped with radiation sensors. Next week we will share the results of our first flight from a launch site in Chile. Stay tuned! Realtime Space Weather Photo Gallery SPRINGTIME IN ANTARCTICA: Spring has begun in Antarctica, and the skies are turning green. No wonder overwintering researchers are taking off their parkas and going outside. B. Sudarsan Patro took this picture on October 1st from the Bharati Indian Base Station in the Larsemann Hills: "The view was absolutely amazing,"says Patro. "The auroras were so bright and colorful. They brought joy to our celebration of Navaratri." Navaratri is a festival dedicated to the worship of the Hindu deity Durga. Technically, it begins on Oct. 2nd, but Patro and colleagues got an early start. The festival lasts 9 days. Earth is passing through an unusually broad stream of solar wind, so a fair fraction of the celebration could be attended by Southern Lights. As October begins, the solar wind around Earth is blowing almost 600 km/s (1.3 million mph). This could spark auroras around both poles this weekend. Monitor the gallery for sightings: Realtime Aurora Photo Gallery Realtime Sprite Photo Gallery | Cosmic Rays in the Atmosphere | Updated: Sept. 29 2016 // Next Flight: Oct. 1, 2016 Sept. 20, 2016: 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 12% 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. 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 Oct. 1, 2016, the network reported 20 fireballs. (19 sporadics, 1 Southern Taurid) 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] 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 October 1, 2016 there were potentially hazardous asteroids. 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. | The official U.S. government space weather bureau | | The first place to look for information about sundogs, pillars, rainbows and related phenomena. | | Researchers call it a "Hubble for the sun." 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