Thursday, July 04, 2013

NASA | First X-Class Solar Flares of 2013




Published on May 13, 2013
On May 12-13 the sun erupted with an X1.7-class and an X2.8-class flare as well as two coronal mass ejections, or CMEs, off the upper left side of the sun. Solar material also danced and blew off the sun in what's called a prominence eruption, both in that spot and on the lower right side of the sun. This movie compiles imagery of this activity from NASA's Solar Dynamics Observatory and from the ESA/NASA Solar Heliospheric Observatory.

Music: "Long Range Cruise" by Lars Leonhard, courtesy of the artist and BineMusic. www.lars-leonhard.de


This video is public domain and can be downloaded at: http://svs.gsfc.nasa.gov/vis/a010000/...

Wednesday, July 03, 2013

Consciousness, as a Biophotonic System

The structure of optical radiation emitted by the samples of loach fish eggs is studied. It was found earlier that such radiation perform the communications between distant samples, which result in the synchronization of their development. The photon radiation in form of short quasi-periodic bursts was observed for fish and frog eggs, hence the communication mechanism can be similar to the exchange of binary encoded data in the computer nets via the noisy channels. The data analysis of fish egg radiation demonstrates that in this case the information encoding is similar to the digit to time analogue algorithm. Photonic Communications and Information Encoding in Biological Systems
Of course there is some difficulty by assigning life in human form as an assumption of coordinating a life form system based entirely on computerized processes. But at the same time, there has been this struggle with coordinating the idea behind color of gravity and sonification maturation with the basis of understanding the emotive system as part of the communicating system of our experience.

 The term biophotonics denotes a combination of biology and photonics, with photonics being the science and technology of generation, manipulation, and detection of photons, quantum units of light. Photonics is related to electronics and photons.Photons play a central role in information technologies such as fiber optics the way electrons do in electronics.

So definitely,  I would want some physical process that would emulate the sensitivity with which any detector would be present in the determination of those emotions present in the system at any time during any experience.

Nobody is quite sure how cells produce biophotons but the latest thinking is that various molecular processes can emit photons and that these are transported to the cell surface by energy carying excitons. A similar process carries the energy from photons across giant protein matrices during photosynthesis. Biophoton Communication: Can Cells Talk Using Light?

The very topic(biophotonics) while verging on the one side of mysticism, it begs for sensor development processes that would delve deeper into our psychological makeup and physiological processes,  to bring understanding to the human form and endocrine system as a messenger conduit for such communications?

So of course there are many difficulties in recognizing that consciousness itself would speak too, The Photon and Emergence, suffice it is to say that, consciousness could include emotive forces that are derived from such biophoton messengers that help to define the experience?  So this in a way is a starting point for me about what such science may reveal, that we could say such psychological experiences have definitive facets in the spectrum of observation that we are not currently cataloging?





TEDx Brussels 2010 - Stuart Hameroff - Do we have a quantum Soul?

Monday, July 01, 2013

Off to Vancouver Island



We are returning to the Vancouver Island for some Rest and Relaxation. I will probably be posting from there. This time we will be with  my whole clan. My three adult children, and my 8 grandchildren.

Kye Bay


Kye Bay



Parksville



Qualicum Beach

Courtenay




See:

Kepler-22b

This diagram compares our own solar system to Kepler-22, a star system containing the first "habitable zone" planet discovered by NASA's Kepler mission. The habitable zone is the sweet spot around a star where temperatures are right for water to exist in its liquid form. Liquid water is essential for life on Earth.

Kepler-22's star is a bit smaller than our sun, so its habitable zone is slightly closer in. The diagram shows an artist's rendering of the planet comfortably orbiting within the habitable zone, similar to where Earth circles the sun. Kepler-22b has a yearly orbit of 289 days. The planet is the smallest known to orbit in the middle of the habitable zone of a sun-like star. It's about 2.4 times the size of Earth.
Image credit: NASA/Ames/JPL-Caltech

Kepler Mission Manager Update - 503 New Planet Candidates





Kepler-22b is an extrasolar planet orbiting G-type star Kepler-22.[7][8] It is located 600 light years away from Earth in the constellation of Cygnus. It was discovered by NASA's Kepler Space Telescope in 2011 and was the first known transiting planet to orbit within the habitable zone of a Sun-like star.[7][8]

Songs of the Stars: the Real Music of the Spheres

http://www.perimeterinstitute.ca/videos/songs-stars-real-music-spheres

Songs of the Stars: the Real Music of the Spheres

Recording Details Speaker(s): Donald Kurtz
Collection/Series: Perimeter Institute Public Lecture Series
Perimeter Institute Recorded Seminar Archive (PIRSA).


Different oscillation modes penetrate to different depths inside a star.


Asteroseismology (from Greek ἀστήρ, astēr, "star"; σεισμός, seismos, "earthquake"; and -λογία, -logia) also known as stellar seismology[1][2] is the science that studies the internal structure of pulsating stars by the interpretation of their frequency spectra. Different oscillation modes penetrate to different depths inside the star. These oscillations provide information about the otherwise unobservable interiors of stars in a manner similar to how seismologists study the interior of Earth and other solid planets through the use of earthquake oscillations.[2]

Asteroseismology provides the tool to find the internal structure of stars. The pulsation frequencies give the information about the density profile of the region where the waves originate and travel. The spectrum gives the information about its chemical constituents. Both can be used to give information about the internal structure. Astroseismology effectively turns tiny variations in the star's light into sounds.[3]


Contents

Oscillations

The oscillations studied by asteroseismologists are driven by thermal energy converted into kinetic energy of pulsation. This process is similar to what goes on with any heat engine, in which heat is absorbed in the high temperature phase of oscillation and emitted when the temperature is low. The main mechanism for stars is the net conversion of radiation energy into pulsational energy in the surface layers of some classes of stars. The resulting oscillations are usually studied under the assumption that they are small, and that the star is isolated and spherically symmetric. In binary star systems, stellar tides can also have a significant influence on the star's oscillations. One application of asteroseismology is neutron stars, whose inner structure cannot be directly observed, but may be possible to infer through studies of neutron-star oscillations.[citation needed]


Wave types


Waves in sun-like stars can be divided into three different types;[4]
  • p-mode: Acoustic or pressure (p) modes,[2] driven by internal pressure fluctuations within a star; their dynamics being determined by the local speed of sound.
  • g-mode: Gravity (g) modes, driven by buoyancy,[5]
  • f-mode: Surface gravity (f) modes, akin to ocean waves along the stellar surface.[6]
Within a sun-like star, such as Alpha Centauri, the p-modes are the most prominent as the g-modes are essentially confined to the core by the convection zone. However, g-modes have been observed in white dwarf stars.[5]


Solar seismology


Helioseismology, also known as Solar seismology, is the closely related field of study focused on the Sun. Oscillations in the Sun are excited by convection in its outer layers, and observing solar-like oscillations in other stars is a new and expanding area of asteroseismology.

Space missions


A number of active spacecraft have asteroseismology studies as a significant part of their mission.
  • MOST – A Canadian satellite launched in 2003. The first spacecraft dedicated to asteroseismology.
  • COROT – A French led ESA planet-finder and asteroseismology satellite launched in 2006
  • WIRE – A NASA satellite launched in 1999. A failed infrared telescope now used for asteroseismology.
  • SOHO – A joint ESA / NASA spacecraft launched in 1995 to study the Sun.
  • Kepler – A NASA planet-finder spacecraft launched in 2009 that is currently making asteroseismology studies of over a thousand stars in its field, including the now well-studied subgiant KIC 11026764.[7][8]

Red giants and asteroseismology


Red giants are a later stage of evolution of sun-like stars after the core hydrogen fusion ceases as the fuel runs out. The outer layers of the star expand by about 200 times and the core contracts. However, there are two different stages, first one when there is fusion of hydrogen in a layer outside the core, but none of helium in the core, and then a later stage when the core is hot enough to fuse helium. Previously, these two stages could not be directly distinguished by observing the star's spectrum, and the details of these stages were incompletely understood. With the Kepler mission, asteroseismology of hundreds of relatively nearby red giants[9] enabled these two types of red giant to be distinguished. The hydrogen-shell-burning stars have gravity-mode period spacing mostly ~50 seconds and those that are also burning helium have period spacing ~100 to 300 seconds. It was assumed that, by conservation of angular momentum, the expansion of the outer layers and contraction of the core as the red giant forms would result in the core rotating faster and the outer layers slower. Asteroseismology showed this to indeed be the case[10] with the core rotating at least ten times as fast as the surface. Further asteroseismological observations could help fill in some of the remaining unknown details of star evolution.


References

  1. ^ Ghosh, Pallab (23 October 2008). "Team records 'music' from stars". BBC News. Retrieved 2008-10-24.
  2. ^ a b c Guenther, David. "Solar and Stellar Seismology". Saint Mary's University. Retrieved 2008-10-24.
  3. ^ Palmer, Jason (20 February 2013). "Exoplanet Kepler 37b is tiniest yet - smaller than Mercury". BBC News. Retrieved 2013-02-20.
  4. ^ Unno W, Osaki Y, Ando H, Saio H, Shibahashi H (1989). Nonradial Oscillations of Stars (2nd ed.). Tokyo, Japan: University of Tokyo Press.
  5. ^ a b Christensen-Dalsgaard, Jørgen (June 2003). "Chapter 1" (PDF). Lecture Notes on Stellar Oscillations (5th ed.). p. 3. Retrieved 2008-10-24.
  6. ^ Christensen-Dalsgaard, Jørgen (June 2003). "Chapter 2" (PDF). Lecture Notes on Stellar Oscillations (5th ed.). p. 23. Retrieved 2008-10-24.
  7. ^ Metcalfe, T. S.; et al (2010-10-25). "A Precise Asteroseismic Age and Radius for the Evolved Sun-like Star KIC 11026764". The Astrophysical Journal 723 (2): 1583. arXiv:1010.4329. Bibcode:2010ApJ...723.1583M. doi:10.1088/0004-637X/723/2/1583.
  8. ^ "Graphics for 2010 Oct 26 webcast – Images from the Kepler Asteroseismology Science Consortium (KASC) webcast of 2010 Oct 26". NASA. 2010-10-26. Retrieved 3 November 2010.
  9. ^ Bedding TR, Mosser B, Huber D, Montalbaan J, et al. (Mar 2011). "Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars". Nature 471 (7340): 608–611. arXiv:1103.5805. Bibcode:2011Natur.471..608B. doi:10.1038/nature09935. PMID 21455175.
  10. ^ Beck, Paul G.; Montalban, Josefina; Kallinger, Thomas; De Ridder, Joris; et al. (Jan 2012). "Fast core rotation in red-giant stars revealed by gravity-dominated mixed modes". Nature 481 (7379): 55–57. arXiv:1112.2825. Bibcode:2012Natur.481...55B. doi:10.1038/nature10612. PMID 22158105.

 

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Friday, June 28, 2013

NASA | IRIS: The Science of NASA's Newest Solar Explorer



At the end of June 2013, NASA will launch its newest mission to watch the sun: the Interface Region Imaging Spectrograph, or IRIS. IRIS will show the lowest levels of the sun's atmosphere, the interface region, in more detail than has even been observed before. This will help scientists understand how the energy dancing through this area helps power the sun's million-degree upper atmosphere, the corona, as well as how this energy powers the solar wind constantly streaming off the sun to fill the entire solar system.

Data visualizations courtesy of Mats Carlsson and Viggo Hansteen, University of Oslo, Norway

This video is public domain and can be downloaded at: http://svs.gsfc.nasa.gov/goto?1125611



See:

Eben Moglen: The alternate net we need, and how we can build it.....

Tuesday, June 25, 2013

Iris-Interface Region Imaging Spectrograph

This graphic shows the IRIS observatory with the solar arrays removed. The orange section to the left is the spacecraft bus which includes the spacecraft support structure, the command and data handling system, power distribution system, reaction wheels, X- and S-Band communications systems, Li-Ion battery, magnetic torque rods, and electronics for the sun sensors. The section to the right of the spacecraft includes the instrument optics package and electronics, several components of the attitude control system, and the solar arrays. The instrument includes a 20cm telescope optimized for solar observations which feeds a 5 channel imaging spectrograph. The green section is the telescope assembly, the light blue section is the spectrograph, and the dark blue box is the separate instrument electronics box. Credit: LMSAL, LM ATC


NASA is getting ready to launch a new mission, a mission to observe a largely unexplored region of the solar atmosphere that powers its dynamic million-degree outer atmosphere and drives the solar wind. In late June 2013, the Interface Region Imaging Spectrograph, or IRIS, will launch from Vandenberg Air Force Base, Calif. IRIS will advance our understanding of the interface region, a region in the lower atmosphere of the sun where most of the sun's ultraviolet emissions are generated. Such emissions impact the near-Earth space environment and Earth's climate. See:IRIS: Studying the Energy Flow that Powers the Solar Atmosphere

This image shows the Heliophysics System Observatory (HSO). The HSO utilizes the entire fleet of solar, heliospheric, geospace, and planetary spacecraft as a distributed observatory to discover the larger scale and/or coupled processes at work throughout the complex system that makes up our space environment. The HSO consist of 18 operating missions: Voyager, Geotail, Wind, SOHO, ACE, Cluster, TIMED, RHESSI, TWINS, Hinode, STEREO, THEMIS, AIM, CINDI, IBEX, SDO, ARTEMIS, Van Allen Probes Credit: NASA

Thursday, June 20, 2013

Olay to Divine Inspiration

I think one needs to draw a distinction here with regard to what consciousness is able to access, given the understanding that information already exists. That becoming aware of it, as part and parcel of something larger then ourselves.....as in the conscious state access versus the unconscious ability and doorway too.

Anyway, I presented the Dialogues of Plato and the Plays of William Shakespeare as forums in which characters real or imagined, help to move forward the reader under "ideological progressions," as if,  dealing with this inductive/ deductive realization of information and probable outcomes once given the scenarios which are displayed for the mind to entertain Understanding our Angels and Daemons

While one gets to the point of what is self evident, and lays the point or question as a point of gaining access to that information, how does one see this conscious intent, as it gains access to levels of perception becoming fully aware of "other entities(Gateway Program)," versus, access to information in terms of the collective unconscious? Everything is information, and information, is not lost.


   Elizabeth Gilbert muses on the impossible things we expect from artists and geniuses -- and shares the radical idea that, instead of the rare person "being" a genius, all of us "have" a genius. It's a funny, personal and surprisingly moving talk.

    The author of Eat, Pray, Love, Elizabeth Gilbert has thought long and hard about some large topics. Her next fascination: genius, and how we ruin it.Elizabeth Gilbert on nurturing creativity

The question arises in my mind with regard to seeing these entities as being apart from oneself(Daemon) not Demon:) and gaining access to the same information exhibited in recognition of this higher intelligence that already exists in us all?? Are you aware of the content of "deep play?"


    The words daemon, dæmon, are Latinized spellings of the Greek δαίμων (daimôn),[1] used purposely today to distinguish the daemons of Ancient Greek religion, good or malevolent "supernatural beings between mortals and gods, such as inferior divinities and ghosts of dead heroes" (see Plato's Symposium), from the Judeo-Christian usage demon, a malignant spirit that can seduce, afflict, or possess humans See:Daemon (mythology)

I try to elaborate more here. So it was more that we loose something of ourselves when we see the nature of "an entity" as something apart from ourselves as we consciously push the boundaries of information access. I give two examples with regard too, Robert Pirsig and John Nash. More the fear then,  that such genius is associated with illness and that with this creative spark, and assumed so?

This understanding is a foundational perspective that Socrates may have shared as he intently listened to people. He was looking for this ability of people to access and use this aspect of them self. To express aspect of this higher intelligence? Historically then, the understanding and development of the Socratic foundations? Here my view may be skewed by what is mythical as Gilbert portrays of Socratic as to "a being" inside of us, while I intend to show a development of knowledge pursue.

So herein lies the difficulties I am facing with regard to TC.

Sunday, June 16, 2013

Freeman Dyson: 98 - Summer school at Les Houches



Born in England in 1923, Freeman Dyson moved to Cornell University after graduating from Cambridge University with a BA in Mathematics. He subsequently became a professor and worked on nuclear reactors, solid state physics, ferromagnetism, astrophysics and biology. He has published several books and, among other honours, has been awarded the Heineman Prize and the Royal Society's Hughes Medal. See:98-Summer school at Les Houches



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