On the other hand, the 19th century observations is based on only counted easily
observed sunspots, so we may be below the older trend, since we're now counting Tiny Tims.
The leading `' Skeptics» realized that: it's easier with a telescope to see distant objects in details - > concocted that: Galileo, and after him, people were
observing the sunspots.
DOUBLE CON IS BETTER The leading `' Skeptics» realized that: it's easier with a telescope to see distant objects in details - > concocted that: Galileo, and after him, people were
observing the sunspots.
Of particular interest is the AGU Conference «poster» for «A Decade of Diminishing Sunspot Vigor» http://www.leif.org/research/Livingston-Poster.jpg Within this, there is a graph «Ratio
Observed Sunspot Number to SSN from F10.7».
The observed sunspot number (SSN) was merely 5.7, which is only 14 % of what is typically normal for month number 108 into the cycle.
Not exact matches
Sunspots have been
observed for more than two thousand years, but in the seventeenth century, astronomers devised new ways to view them, including a telescope - based projection device known as a helioscope.
In 1859, astronomer Richard Carrington
observed strange
sunspots — evidence of the largest geomagnetic storm in history — later reproduced in a sketch.
So far this has been the best way to
observe the surface structures of distant stars, but there may be misinterpretations, so there have been doubts about the accuracy concerning the existence of the polar
sunspots.
Now astrophysicists from the Niels Bohr Institute have
observed a distant star in the constellation Andromeda with a different positioning of
sunspots and this indicates a magnetic field that is driven by completely different internal dynamics.
«What we can
observe on the star is that it has a large
sunspot at its north pole.
On our star, the Sun, the
sunspots are seen in a belt around the equator, but now scientists have
observed a large, distant star where
sunspots are located near the poles.
Astronomers have previously seen
sunspots on Zeta Andromeda using the Doppler method, which means that you
observe that light wavelengths of the rotating star.
Two flat mirrors and an objective lens atop the tower catch the sun's image and toss it down a tube to the ground - level
observing room, where the
sunspot drawings are made.
How do you figure out what powers solar flares — the intense bursts of radiation coming from the release of magnetic energy associated with
sunspots — when you must rely on
observing only the light and particles that make their way to near - Earth's orbit?
From 1645 to 1715, a period known as the Maunder Minimum, there were virtually no
sunspots observed, indicating a «quiet» period in the sun's activity.
Another team led by William Livingston, also of the National Solar Observatory, has
observed magnetic fields necessary to produce
sunspots steadily weakening for the past 13 years.
Microwaves have the advantage that, unlike
sunspots, they can be
observed on cloudy days.
He first used it to
observe the moon and see the shadows cast by its mountains and craters; he went on to catalogue
sunspots; and he discovered the four largest moons of Jupiter — Io, Europa, Ganymede and Callisto — that are now known as the Galilean moons in his honor.
Crucially, the same pattern has been
observed over two
sunspot cycles.
Drawing by Valderrama of the solar flare he
observed on 10 September 1886 on a
sunspot (with the penumbra shown with hashed lines and the umbra in black).
This meant the team could make hundreds of detailed observations of each shock wave by
observing how it distorted the pattern of
sunspots.
What they found came as a surprise: As the object rotated, a powerful magnetic region came into view, more powerful than the magnetic fields associated with
sunspots that we
observe on the sun.
The gigantic
sunspot in the upper left of this image is about 50,000 miles (80,000 km) long and was
observed on the sun by NASA's Solar Dynamics Observatory on Nov. 3, 2011.
Using LOS magnetograms, the authors
observed a small region of transient polarity - reversed magnetic field in the main
sunspot of NOAA 11429 on 13 March 2012, which corresponded with flare brightenings seen in intensity images.
This large field - of - view image of
sunspots in Active Region 10030 was
observed on July 15, 2002.
Probably the largest
sunspot that we have
observed in several years has rotated to the center of the Sun (Nov. 6 - 8, 2011) as viewed by SDO where effects from solar storms could possibly be felt here at Earth.
When
observing the Sun with appropriate filtration, the most immediately visible features are usually its
sunspots, which are well - defined surface areas that appear darker than their surroundings due to lower temperatures.
Changing a cartridge, opening the enclosure, sunset, and nightly
observing at the Sloan Foundation 2.5 m Telescope at Apache Point Observatory,
Sunspot, New Mexico.
At Parkland Magnet Middle School for Aerospace Technology on April 18, Mr. Bush watched a 6th grade class use robotic arms to pick up balls, saw students using technology to trace
sunspots, and
observed scientists from the space agency guiding students» studies.
More than 95 % of the 5 yr running mean of the surface temperature change since 1850 can be replicated by an integration of the
sunspot data (as a proxy for ocean heat content), departing from the average value over the period of the
sunspot record (~ 40SSN), plus the superimposition of a ~ 60 yr sinusoid representing the
observed oceanic oscillations.
Actually, the discovery of the Maunder Minimum should be attributed to the French astronomer Jean - Jacques Dortous de Mairan (1678 - 1771), who reported a link between solar activity, based on the abundance of
sunspots, and the frequency of aurorae
observed at mid-latitudes (e.g. in Paris or Montpellier).
Sunspot observations for the last 400 years clearly indicate that current levels of solar activity are very different from the state of the sun during the Maunder minimum (from approx. 1645 to 1715 AD) where almost no
sunspots could be
observed.
British astronomer William Herschel
observed in 1801, a direct correlation between the historical record of
sunspots and grain prices — indicating that the solar cycles do have a strong impact on climate variability.
There is a couple tenths of a W / m2 of long - term solar forcing (warming) that is inferred the
observed changes in the
sunspot cycle (which we include in our climate simulations, including the UV variations).
Before that, for 100y they were blocking the sun with a cardboard and
observing the sun - flare; NOT
sunspots!!!
Abstract It has been suggested recently that early
sunspot numbers should be re-calibrated and significantly corrected using the
observed daily range of the geomagnetic declination (so - called rY values).
Concentrating here on Zürich
sunspot numbers (Rz), we demonstrate that the rY values do not actually imply that the
observed Rz values in the 19th century are systematically underestimated.
They noted that empirical models based upon
sunspots and faculae do not account for all irradiance variations
observed over an activity cycle (see also NRC (1994)-RRB- and base their con - elation on an
observed relationship between brightness and excess chromospheric emission, using the Ca II H and...»
http://arxiv.org/abs/1009.0784v1 Long - term Evolution of
Sunspot Magnetic Fields Independent of the normal solar cycle, a decrease in the sunspot magnetic field strength has been observed using the Zeeman - split 1564.8 nm Fe I spectral line at the NSO Kitt Peak McMath - Pierce tel
Sunspot Magnetic Fields Independent of the normal solar cycle, a decrease in the
sunspot magnetic field strength has been observed using the Zeeman - split 1564.8 nm Fe I spectral line at the NSO Kitt Peak McMath - Pierce tel
sunspot magnetic field strength has been
observed using the Zeeman - split 1564.8 nm Fe I spectral line at the NSO Kitt Peak McMath - Pierce telescope.
This has been directly
observed using space - borne measurements of TSI during times of transit of
sunspots across the visible solar disk.
The Babcock Model describes a mechanism which can explain magnetic and
sunspot patterns
observed on the Sun.
In this study, we address the question of whether the
observed decrease in the TSI is the result of evolving solar surface magnetism (
sunspots and faculae).
If an expert has identified a 420 year long solar cycle and we have only been looking as
sunspots for about 400 years (since the invention of the telescope in 1608) that would mean that this person has
observed less than one full cycle of information?
Thus your assertion is moot because regardless of whether
sunspot counts in the more distant past are accurate we know for a fact there was a recent transition of large magnitude so we will still be able to
observe what happens when
sunspot count changes radically.
Almost no
sunspots were
observed during a 70 - y interval (1645 — 1715) called the Maunder Minimum (1).
A simple numerical model using known
sunspots and known PDO changes and a 22 year lag time produces the
observed temperature trends since 1900.
Re # 57: Let me answer with this google - quote: «IT is now more than 200 years since the great astronomer William Herschel
observed a correlation between wheat prices and
sunspots.
With more than 13 years of
sunspot data collected at the McMath - Pierce Telescope at Kitt Peak in Arizona, Matt Penn and William Livingston
observed that the average magnetic field strength declined significantly during Cycle 23 and now into Cycle 24.
Other quotes from your article: «He says that the increased solar brightness over the past 20 years has not been enough to cause the
observed climate changes» «While the established view remains that the sun can not be responsible for all the climate changes we have seen in the past 50 years or so, this study is certainly significant,» «He added, however, that the study also showed that over the past 20 years the number of
sunspots had remained roughly constant, while the Earth's temperature had continued to increase.»
Sunspots have been
observed for millennia, first in China and with a telescope for the first time by Galileo in 1610.