SOLAR VELOCITY
Defenders of truth, justice and effective marketing, the Solar Velocity team is a diverse group of highly talented individuals all born with special marketing powers. Our mission: to save the galaxy, one client at a time, Over ten years ago we heard cries of distress coming from beleaguered businesses and decided to take action. Operating out of our office of solitude in Atlanta, Georgia, we make the most of cutting edge website design, social media, search marketing, and web / mobile developmen... t to help innocent businesses defend themselves against villainous competition. Comprised of the best and the brightest, each member of the Solar Velocity team is recognized for their love of the digital solar system and drive to finish first. We have recruited a new generation of strategic and creative leaders into our ranks and our numbers grow as highly qualified professionals armed with fresh perspectives continue to join our cause. Specialties Social CRM Strategies, Social Media, Digital Marketing, Web Development, Web Design, Mobile Development, Content Management Systems, Email Marketing, Search Marketing
SOLAR VELOCITY
Industry:
Advertising Consulting CRM Digital Marketing Mobile Apps Social Media Software Web Design Web Development
Founded:
1999-01-01
Address:
Smyrna, Georgia, United States
Country:
United States
Total Employee:
11+
Status:
Active
Founder
More informations about "Solar Velocity"
Alfvénic velocity spikes and rotational flows in the near-Sun solar ...
Dec 4, 2019 Data collected by the Parker Solar Probe in the solar corona are used to determine the organization of Alfvén waves, revealing an increasing flow velocity peaking at โฆSee details»
On the Solar Velocity - IOPscience
Nov 13, 2018 The American Astronomical Society (AAS), established in 1899 and based in Washington, DC, is the major organization of professional astronomers in North America. Its membership of about 7,000 individuals also includes physicists, mathematicians, geologists, โฆSee details»
Solar Velocity - Crunchbase Company Profile & Funding
Defenders of truth, justice and effective marketing, the Solar Velocity team is a diverse group of highly talented individuals all born with special marketing powers. Our mission: to save the galaxy, one client at a time, Over ten years โฆSee details»
Connecting Solar Wind Velocity Spikes Measured by Solar Orbiter โฆ
Jun 19, 2024 Second, since velocity spikes are Alfvénic perturbations and the propagation speed of the switchbacks in the solar wind flow reference frame is approximately the local โฆSee details»
Reconstructing Synoptic Maps of Solar Wind Radial Velocity โฆ
May 30, 2023 We also find that the radial solar wind velocity from the synoptic map matches well with in situ observations from Wind and STEREO-A/B near 1 au. Half of the compared solar โฆSee details»
Solar Wind Plasma Particles Organized by the Flow Speed - Springer
Bi-modal organization of the solar wind may need more re๏ฌned complementary data analy-sis for understanding and identifying the sources of solar wind (Stansby et al., 2018;Berciห หc ... The โฆSee details»
Multiscale views of an Alfvénic slow solar wind: 3D velocity ...
Precise kinetic organization of the plasma, thus, to measure the velocity distribution functions (VDF) of the di erent species, at the relevant scales. These measurements, for the proton and โฆSee details»
The local standard of rest from data on young objects with โฆ
To estimate the peculiar velocity of the Sun with respect to the local standard of rest (LSR), we used young objects in the Solar neighbourhood with distance measurement errors within โฆSee details»
Multiscale views of an Alfvénic slow solar wind: 3D velocity ...
For the whole period, their cross-correlation is โผ0.94. The overall organization along a slope โผ0.65 is obvious. This is less than 1 (the expected slope for strict Alfvénic disturbances). ...See details»
On the Solar Velocity - NASA/ADS
Adshelp[at]cfa.harvard.edu The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86ASee details»
Direct observations of a complex coronal web driving highly
Nov 24, 2022 Historically, the solar wind 1 has been categorized as โfastโ or โslowโ wind. The fast wind is generally described as having speeds greater than 500 km s โ1 and originating from โฆSee details»
First Solar Orbiter observation of the Alfvénic slow wind and ...
3. Global in situ description of the stream. Although the Alfvénic slow wind has mainly been observed and studied during the maximum of the solar cycle, evidence of the presence of this โฆSee details»
The distribution of solar wind speeds during solar โฆ
Mar 1, 2011 [1] It took the solar polar passage of Ulysses in the early 1990s to establish the global structure of the solar wind speed during solar minimum. However, it remains unclear if the solar wind is composed of two distinct โฆSee details»
On Alfvénic Slow Wind: A Journey From the Earth Back โฆ
Mar 22, 2021 Furthermore, DโAmicis, Matteini, and Bruno found that, in both fast and slow Alfvénic winds, a well-defined correlation exists between the proton speed and the cosine of the angle between the magnetic field and the solar โฆSee details»
An Alternative Approach to Measuring Solar Velocities on the Solar ...
Weighted velocity at each pixel, making the velocity estimate robust against gain errors (good!) 2. Needs of additional calibration via a sensitivity curve that assumes how the spectral line looks like at each pixel (bad!) This HMI method is causing a leak of the spacecraft velocity (a known quantity) on the solar data.See details»
Solar Rotation and Its Gradient - IOPscience
For the solar dynamo models, however, spatial gradients of this angular velocity are more important. Although the radial gradient of the rotation rate in the outer shear layer has been โฆSee details»
Solar wind Alfvénicity during solar cycle 23 and 24
Oct 19, 2021 Alfvénicity is a feature of solar wind fluctuations frequently observed in interplanetary data. It is characterized by a strong correlation between velocity and magnetic โฆSee details»
orbital mechanics - Calculating solar system escape and and sun โฆ
Again, the trip is broken up into 3 segments according to my organization, but the last 2 are really the same burn. Let me focus on the escape from our solar system. The three legs are: A โฆSee details»
Global-scale equatorial Rossby waves as an essential component โฆ
May 7, 2018 Figure 1 shows maps of the horizontal vector velocity (arrows) and the radial component of the vorticity (background colours) for three consecutive solar rotation periods โฆSee details»
Multiscale views of an Alfvénic slow solar wind: 3D velocity ...
Dec 1, 2021 The Alfvénic slow solar wind is of particular interest, as it is often characterized by intense magnetic turbulence, complex proton 3D velocity distribution functions (VDF), and an โฆSee details»