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Dr Michael
- Rate R219
- Response 1h

R219/h
Unfortunately, this tutor is not available
- Maths
- Physics
- School science
Mature PhD adult tutors first level of computational Astrophysics for anyone interested in gaining insight into the methods used for understanding the physical properties of the Sun ranging from tempe
- Maths
- Physics
- School science
Lesson location
About Dr Michael
I am a retired softy (last job banking software) have a first class degree Physics/Maths PhD in Astrophysics published 4 papers (one in Nature Kiraly et al 1975 vol 255 p 619-20) and as a result of the two-way process of teaching (encouraging the right questions) there's nothing to stop anyone from publishing novel aspects of understanding or data analysis ,resulting from 1-1 consultation or formation a small team of like-minded people which could achieve great things.
Currently I am trying to integrate a dynamo model with temp models of the Sun, and numerically experiment with deviatons from sphericity,namely oblate spheroidal coords ( used for galaxies).
If all this sounds complicated the do not worry since Boltzmann's equa E=kT relating thermodynamics tquantum mechanics E=hf h Planck's constant ,f or nu frequency of particle is a flying start!
About the lesson
- Primary
- Secondary
- Matric/GCSE
- +9
levels :
Primary
Secondary
Matric/GCSE
AS Level
A Level
BTech
Adult education
Undergraduate
Masters
Diploma
Doctorate
MBA
- English
Languages in which the lesson is available :
English
Whilst doing My PhD thesis I gained 2 years experience of providing physics theory solutions to a small group of students each week. my approach is to scale this down to be more individually orientated either online ( zoom) or for locals in my spare tutoring room equipped with a small telescope + computers for when needed.
I am hoping that a series of 6 1/2hr lessons will firstly explain to a sufficient degree stellar evolution & nucleosynthesis progressing to supernovae,neutron stars & black holes. Then the fun starts with the studentbeing empowered to produce an software model/app of temperature distribution in the Sun, or gaLactic collisions-Andromedra is approaching ! These are optional lessons 7 -10 requireing someknowledge of a computer language such as BASIIC,FORTRAN,c OR c++ .
Rates
Rate
- R219
Package rates
- 5h: R1095
- 10h: R2190
online
- R219/h
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