scholarly journals Development of Multi-tasking, Multi-powered Machine for Agriculture Purpose

2021 ◽  
pp. 284-293
Author(s):  
Kadole Pavan Prabhakar ◽  
Bharath Raj H K ◽  
D Yogeshwar Naidu ◽  
G Tharun Sai ◽  
Manjunath R
Keyword(s):  
Current Method ◽  
Current Situation ◽  
The Sun ◽  
Oriented Energy ◽  
Limited Scope

At present famers pay a lot of money on machines that work with them decline work and increment yield of harvests. The Multipurpose machine is accustomed to planting the seeds and manure shower into land and seed planting for making heaps of plant creation in rural field. It is a mechanical gadget here no electrical or other force source is not needed. The expense of this machine is low and simple to work straightforward in development. As there is huge advancement in the field of designing the current situation makes us to discover answer for serious issues looked by the farming field. The agrarian business is behind elective reciprocal ventures in exploitation robots because of the sort of occupations worried in agribusiness are no and burrow. The fundamental target of this task is to improve the current method of cultivating by presenting multipurpose gear. The greater part of the Farmers in India is affordable frail because of which they cannot buy work vehicles and other expensive hardware's subsequently they utilize conventional strategy for cultivating. This will not fulfill need of energy necessity of the cultivating when contrasted with different nations on the planet. So, work has been completed to plan and manufacture a multipurpose agribusiness vehicle, to perform rural tasks like furrowing, seed planting and showering of pesticides or water utilizing the sun-oriented energy. Likewise in the place of human and animal endeavors can be supplanted by this component of machine which will be reasonable for limited scope rancher from efficient and exertion perspective. So, we are fostering this gear which will fulfill this need and to tackle work issues.

Astrology for Maecenas

Antichthon ◽  
1982 ◽  
Vol 16 ◽  
pp. 88-96
Author(s):  
D.A. Kidd
Keyword(s):  
Special Interest ◽  
The Sun ◽  
Julian Calendar ◽  
Time Of Year ◽  
A Minor ◽  
Limited Scope

Astronomical themes, with a rather limited scope, were a minor but recurrent element in ancient poetry, and Horace makes considerable use of them in the Odes. Most of the examples involve risings and settings as guides to the time of year, and most are within the range of the phenomena mentioned in Hesiod’s Works and Days. But in Odes 3.29.17-20, for the special interest of Maecenas, Horace breaks new ground by drawing more topical material from the Julian calendar, to remind his friend that it is now July and too hot for working in Rome: the (evening) rising of Cepheus on the 9th, the (morning) risings of Procyon on the 15th and Regulus on the 29th, and the entry of the sun into Leo on the 17th. Such an array of calendaric lore is clearly designed to appeal to Maecenas, who must have had a particular interest in astronomical phenomena.

scholarly journals O Centro de Turismo de Natal (RN, Brasil): subsídios para o estudo do centro histórico

2021 ◽  
Vol 19 (2) ◽  
pp. 337-353
Author(s):  
Fernando Manuel Rocha da Cruz ◽  
Keyword(s):  
Public Policies ◽  
Rio Grande ◽  
Cultural Tourism ◽  
Current Situation ◽  
The Sun ◽  
Structured Interviews ◽  
Brazilian State ◽  
Historic Centre ◽  
The City

Natal, capital of the Brazilian state of Rio Grande do Norte, annually receives two million tourists, mainly from the sun and beach segment. Its historic centre was classified by Iphan as a Brazilian cultural heri‑ tage in 2010. In this article, we seek to identify the potential and weaknesses of cultural tourism, starting from the historic centre of Natal. To this end, we carried out a case study, from the Tourism Centre, which is located in the aforementioned historic centre. In this context, semi-structured interviews were applied to businessmen, tourism secretaries - municipal and state - and tourists. We conclude that, despite some advances, the historic centre remains in a secondary position in political and economic options. In addition, the triangulation of Natal's culture, tourism and public policies allows the identification of positive and negative skills that make it possible to characterize the current situation of cultural tourism in the city

Chromospheric activity as a function of age in main-sequence stars

1966 ◽  
Vol 24 ◽  
pp. 40-43
Author(s):  
O. C. Wilson ◽  
A. Skumanich
Keyword(s):  
Main Sequence ◽  
The Sun ◽  
Main Sequence Stars ◽  
Tentative Conclusion ◽  
Chromospheric Activity ◽  
General Field ◽  
Large Clusters

Evidence previously presented by one of the authors (1) suggests strongly that chromospheric activity decreases with age in main sequence stars. This tentative conclusion rests principally upon a comparison of the members of large clusters (Hyades, Praesepe, Pleiades) with non-cluster objects in the general field, including the Sun. It is at least conceivable, however, that cluster and non-cluster stars might differ in some fundamental fashion which could influence the degree of chromospheric activity, and that the observed differences in chromospheric activity would then be attributable to the circumstances of stellar origin rather than to age.

Galactic orbits of stars

1966 ◽  
Vol 25 ◽  
pp. 93-97
Author(s):  
Richard Woolley
Keyword(s):  
Globular Cluster ◽  
Potential Field ◽  
High Velocity ◽  
Velocity Vector ◽  
Variable Stars ◽  
The Sun ◽  
Proper Motions ◽  
Rr Lyrae ◽  
The Galaxy

It is now possible to determine proper motions of high-velocity objects in such a way as to obtain with some accuracy the velocity vector relevant to the Sun. If a potential field of the Galaxy is assumed, one can compute an actual orbit. A determination of the velocity of the globular clusterωCentauri has recently been completed at Greenwich, and it is found that the orbit is strongly retrograde in the Galaxy. Similar calculations may be made, though with less certainty, in the case of RR Lyrae variable stars.

Seti Space Missions

1997 ◽  
Vol 161 ◽  
pp. 761-776 ◽  
Author(s):  
Claudio Maccone
Keyword(s):  
Electromagnetic Waves ◽  
Space Missions ◽  
Gravitational Lens ◽  
The Sun ◽  
Space Antenna ◽  
Focal Distance ◽  
Large Space ◽  
The Earth ◽  
Space Antennas ◽  
New Space

AbstractSETI from space is currently envisaged in three ways: i) by large space antennas orbiting the Earth that could be used for both VLBI and SETI (VSOP and RadioAstron missions), ii) by a radiotelescope inside the Saha far side Moon crater and an Earth-link antenna on the Mare Smythii near side plain. Such SETIMOON mission would require no astronaut work since a Tether, deployed in Moon orbit until the two antennas landed softly, would also be the cable connecting them. Alternatively, a data relay satellite orbiting the Earth-Moon Lagrangian pointL2would avoid the Earthlink antenna, iii) by a large space antenna put at the foci of the Sun gravitational lens: 1) for electromagnetic waves, the minimal focal distance is 550 Astronomical Units (AU) or 14 times beyond Pluto. One could use the huge radio magnifications of sources aligned to the Sun and spacecraft; 2) for gravitational waves and neutrinos, the focus lies between 22.45 and 29.59 AU (Uranus and Neptune orbits), with a flight time of less than 30 years. Two new space missions, of SETI interest if ET’s use neutrinos for communications, are proposed.

A Search for Dyson Spheres around Late-Type Stars in the Solar Neighborhood II

1997 ◽  
Vol 161 ◽  
pp. 707-709 ◽  
Author(s):  
Jun Jugaku ◽  
Shiro Nishimura
Keyword(s):  
Solar Neighborhood ◽  
The Sun ◽  
Late Type ◽  
Solar Type

AbstractWe continued our search for partial (incomplete) Dyson spheres associated with 50 solar-type stars (spectral classes F, G, and K) within 25 pc of the Sun. No candidate objects were found.

Emergence of Twisted Magnetic Flux Related Sigmoidal Brightening

2000 ◽  
Vol 179 ◽  
pp. 263-264
Author(s):  
K. Sundara Raman ◽  
K. B. Ramesh ◽  
R. Selvendran ◽  
P. S. M. Aleem ◽  
K. M. Hiremath
Keyword(s):  
Magnetic Field ◽  
Magnetic Fields ◽  
Magnetic Flux ◽  
Ultra Violet ◽  
Active Regions ◽  
Morphological Properties ◽  
Energy Storage And Conversion ◽  
The Sun ◽  
X Rays ◽  
The Magnetic Field

Extended AbstractWe have examined the morphological properties of a sigmoid associated with an SXR (soft X-ray) flare. The sigmoid is cospatial with the EUV (extreme ultra violet) images and in the optical part lies along an S-shaped Hαfilament. The photoheliogram shows flux emergence within an existingδtype sunspot which has caused the rotation of the umbrae giving rise to the sigmoidal brightening.It is now widely accepted that flares derive their energy from the magnetic fields of the active regions and coronal levels are considered to be the flare sites. But still a satisfactory understanding of the flare processes has not been achieved because of the difficulties encountered to predict and estimate the probability of flare eruptions. The convection flows and vortices below the photosphere transport and concentrate magnetic field, which subsequently appear as active regions in the photosphere (Rust & Kumar 1994 and the references therein). Successive emergence of magnetic flux, twist the field, creating flare productive magnetic shear and has been studied by many authors (Sundara Ramanet al.1998 and the references therein). Hence, it is considered that the flare is powered by the energy stored in the twisted magnetic flux tubes (Kurokawa 1996 and the references therein). Rust & Kumar (1996) named the S-shaped bright coronal loops that appear in soft X-rays as ‘Sigmoids’ and concluded that this S-shaped distortion is due to the twist developed in the magnetic field lines. These transient sigmoidal features tell a great deal about unstable coronal magnetic fields, as these regions are more likely to be eruptive (Canfieldet al.1999). As the magnetic fields of the active regions are deep rooted in the Sun, the twist developed in the subphotospheric flux tube penetrates the photosphere and extends in to the corona. Thus, it is essentially favourable for the subphotospheric twist to unwind the twist and transmit it through the photosphere to the corona. Therefore, it becomes essential to make complete observational descriptions of a flare from the magnetic field changes that are taking place in different atmospheric levels of the Sun, to pin down the energy storage and conversion process that trigger the flare phenomena.

Polar Magnetic Field Reversals of the Sun in Maunder Minimum

2000 ◽  
Vol 179 ◽  
pp. 193-196
Author(s):  
V. I. Makarov ◽  
A. G. Tlatov
Keyword(s):  
Magnetic Field ◽  
Maunder Minimum ◽  
The Sun ◽  
Annual Rings ◽  
Field Reversal ◽  
Polar Magnetic Field ◽  
Pine Trees ◽  
Using Data ◽  
Magnetic Field Reversal

AbstractA possible scenario of polar magnetic field reversal of the Sun during the Maunder Minimum (1645–1715) is discussed using data of magnetic field reversals of the Sun for 1880–1991 and the14Ccontent variations in the bi-annual rings of the pine-trees in 1600–1730 yrs.

Solar Filaments as Tracers of Subsurface Processes

2000 ◽  
Vol 179 ◽  
pp. 177-183
Author(s):  
D. M. Rust
Keyword(s):  
Magnetic Fields ◽  
Magnetic Flux ◽  
Coronal Mass Ejections ◽  
Interplanetary Space ◽  
Intermediate Stage ◽  
Coronal Plasma ◽  
Magnetic Helicity ◽  
The Sun ◽  
New Paradigm ◽  
Solar Filaments

AbstractSolar filaments are discussed in terms of two contrasting paradigms. The standard paradigm is that filaments are formed by condensation of coronal plasma into magnetic fields that are twisted or dimpled as a consequence of motions of the fields’ sources in the photosphere. According to a new paradigm, filaments form in rising, twisted flux ropes and are a necessary intermediate stage in the transfer to interplanetary space of dynamo-generated magnetic flux. It is argued that the accumulation of magnetic helicity in filaments and their coronal surroundings leads to filament eruptions and coronal mass ejections. These ejections relieve the Sun of the flux generated by the dynamo and make way for the flux of the next cycle.

Sunspot Groups as Tracers of Sub-Surface Processes

2000 ◽  
Vol 179 ◽  
pp. 155-160
Author(s):  
M. H. Gokhale
Keyword(s):  
Magnetic Flux ◽  
Indian Institute ◽  
Surface Processes ◽  
The Sun ◽  
Global And Local ◽  
Sunspot Groups

AbstractData on sunspot groups have been quite useful for obtaining clues to several processes on global and local scales within the sun which lead to emergence of toroidal magnetic flux above the sun’s surface. I present here a report on such studies carried out at Indian Institute of Astrophysics during the last decade or so.

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