Determination of Patients’ Discharge Learning Needs after Urologic Surgery

Probolinggo Regency is one of the production centers for milkfish producers in East Java. Milkfish has a very good prospect to be developed in the agribusiness especially in fisheries subsector. One of milkfish cultivators group that is known to be active in Probolinggo Regency is Aci Bahari Fish Cultivators Group (Pokdakan). This research aimed to explain the role of Aci Bahari Fish Cultivators Group (Pokdakan) on the cultivation of milkfish in Pesisir Village of Gending District, Probolinggo Regency. The research area was determined by purposive method in Pesisir Village. The research used descriptive qualitative method. Determination of informant conducted by purposive sampling. The methods used in collecting data are interviews, observation, and documentation. Data analysis method used is Miles and Huberman model. The results of the research showed that (1) The role of Aci Bahari Pokdakan as a learning class included the formulation of learning needs, routine group meetings, learning motivation, learning processes and the activeness of the group. (2) The role of Aci Bahari Pokdakan as a vehicle for cooperation included the atmosphere of cooperation, the division of tasks, deliberation of problems, planning of providing production facilities and cooperation with other production parties. (3) The role of Aci Bahari Pokdakan as a production unit included decision making, preparation of the group needs, technology facilities, implementation of group agreements and increasing production sustainability.

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Administrasi husemas

10.31227/osf.io/vsejz ◽

2020 ◽

Author(s):

nurul atika

Keyword(s):

Public Relations ◽

Community Schools ◽

Community Relations ◽

Financial Resources ◽

Learning Needs ◽

Literature Study ◽

Financial Administration ◽

Literature Material

Abstrak- In general, this study aims to determine and analyze the role of school and community relations administration in an education. This research uses the literature study method by collecting literature (material materials) sourced from books, journals, and other sources related to the science of Financial Administration. Public relations administration for a school is a two-way relationship between the school and the community to deliberate on ideas and certain information that is useful for improving education. The benefits of school relations with the community can be described as follows: Determination of sources and learning needs, the availability of places of research, fulfillment of facilities and infrastructure, fulfillment of financial resources and human resources revealed in their creativity, taste, intention and work. Techniques for School Relations with the community: reports to parents, school bulletins, newspapers and school exhibitions. Elements of School Relations with the Community: Schools, Parents of Students, Students and Teachers.

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Administrasi Hubungan Sekolah dan Masyarakat

10.31227/osf.io/d2atf ◽

2019 ◽

Author(s):

Deby Willy Amanda

Keyword(s):

Public Relations ◽

Human Resources ◽

Community Schools ◽

Financial Resources ◽

Learning Needs ◽

School Public Relations

Public relations administration for a school is a two-way relationship between the school and the community to deliberate on ideas and certain information that is useful for improving education. The benefits of school relations with the community can be described as follows: Determination of sources and learning needs, the availability of places of research, fulfillment of facilities and infrastructure, fulfillment of financial resources and human resources revealed in their creativity, taste, intention and work. Techniques for School Relations with the community: reports to parents, school bulletins, newspapers and school exhibitions. Elements of School Relations with the Community: Schools, Parents of Students, Students and Teachers.Public relations administration for a school is a two-way relationship between the school and the community to deliberate on ideas and certain information that is useful for improving education. The benefits of school relations with the community can be described as follows: Determination of sources and learning needs, the availability of places of research, fulfillment of facilities and infrastructure, fulfillment of financial resources and human resources revealed in their creativity, taste, intention and work. Techniques for School Relations with the community: reports to parents, school bulletins, newspapers and school exhibitions. Elements of School Relations with the Community: Schools, Parents of Students, Students and Teachers.Keywords: administration, school, public, relations

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Galactic orbits of stars

Symposium - International Astronomical Union ◽

10.1017/s0074180900105340 ◽

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.

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Distance to SN 1987A and the LMC

Symposium - International Astronomical Union ◽

10.1017/s0074180900118959 ◽

1999 ◽

Vol 190 ◽

pp. 549-554

Author(s):

Nino Panagia

Keyword(s):

Angular Size ◽

Large Magellanic Cloud ◽

Magellanic Cloud ◽

Light Curves ◽

Distance Modulus ◽

Absolute Size ◽

Sn 1987A

Using the new reductions of the IUE light curves by Sonneborn et al. (1997) and an extensive set of HST images of SN 1987A we have repeated and improved Panagia et al. (1991) analysis to obtain a better determination of the distance to the supernova. In this way we have derived an absolute size of the ringRabs= (6.23 ± 0.08) x 1017cm and an angular sizeR″ = 808 ± 17 mas, which give a distance to the supernovad(SN1987A) = 51.4 ± 1.2 kpc and a distance modulusm–M(SN1987A) = 18.55 ± 0.05. Allowing for a displacement of SN 1987A position relative to the LMC center, the distance to the barycenter of the Large Magellanic Cloud is also estimated to bed(LMC) = 52.0±1.3 kpc, which corresponds to a distance modulus ofm–M(LMC) = 18.58±0.05.

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International determination of the total motion of the pole

Symposium - International Astronomical Union ◽

10.1017/s0074180900177824 ◽

1961 ◽

Vol 13 ◽

pp. 29-41

Author(s):

Wm. Markowitz

Keyword(s):

Secular Motion ◽

The Future

A symposium on the future of the International Latitude Service (I. L. S.) is to be held in Helsinki in July 1960. My report for the symposium consists of two parts. Part I, denoded (Mk I) was published [1] earlier in 1960 under the title “Latitude and Longitude, and the Secular Motion of the Pole”. Part II is the present paper, denoded (Mk II).

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Time and Latitude in South Africa

International Astronomical Union Colloquium ◽

10.1017/s0252921100026816 ◽

1972 ◽

Vol 1 ◽

pp. 27-38

Author(s):

J. Hers

Keyword(s):

South Africa ◽

Cape Town ◽

Astronomical Observations ◽

Royal Observatory ◽

The Republic ◽

Astronomical Determination ◽

Limited Accuracy ◽

Better Than

In South Africa the modern outlook towards time may be said to have started in 1948. Both the two major observatories, The Royal Observatory in Cape Town and the Union Observatory (now known as the Republic Observatory) in Johannesburg had, of course, been involved in the astronomical determination of time almost from their inception, and the Johannesburg Observatory has been responsible for the official time of South Africa since 1908. However the pendulum clocks then in use could not be relied on to provide an accuracy better than about 1/10 second, which was of the same order as that of the astronomical observations. It is doubtful if much use was made of even this limited accuracy outside the two observatories, and although there may – occasionally have been a demand for more accurate time, it was certainly not voiced.

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Large-scale Motion of Solar Filaments

International Astronomical Union Colloquium ◽

10.1017/s0252921100064502 ◽

2000 ◽

Vol 179 ◽

pp. 205-208

Author(s):

Pavel Ambrož ◽

Alfred Schroll

Keyword(s):

Magnetic Flux ◽

Proper Motion ◽

Time Scale ◽

Large Scale ◽

Accuracy Of Measurements ◽

Solar Filaments ◽

General Movement ◽

Scale Motion ◽

Velocity Scatter

AbstractPrecise measurements of heliographic position of solar filaments were used for determination of the proper motion of solar filaments on the time-scale of days. The filaments have a tendency to make a shaking or waving of the external structure and to make a general movement of whole filament body, coinciding with the transport of the magnetic flux in the photosphere. The velocity scatter of individual measured points is about one order higher than the accuracy of measurements.

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