M. Shallis

发表

On Time: An Investigation into Scientific Knowledge and Human Experience

M. Shallis, 1982 .

The Silicon Idol: The Micro Revolution and Its Social Implications

M. Shallis, Michael Shallis, 1985 .

Precision measurement of relative oscillator strengths – IX. Measures of Fe I transitions from levels $a^{5} P_{1-3} (2.18-2.28 \,\text{eV}), \,a^{3} \,P_{2} \,(2.28 \,\text{eV}), a{3}\,P_{0,1} \,(2.49-2.42 \,\text{eV}), z^{7}\, D_{1-5}^{0}\, (2.48-2.40 \,\text{eV}) \,\text{and} \,a^{3} \,H_{4-6} \,

G. J. Simmons, M. Shallis, D. Blackwell, 1982 .

Precision measurement of relative oscillator strengths – VIII. Measures of Fe I transitions from levels a3F2–4 (1.49–1.61 eV) with an accuracy of 1 per cent

M. Shallis, D. Blackwell, A. Petford, 1979 .

Interpretation of the solar spectrum 300−900 nm – II. Fe I lines of excitation potential 0.00−1.01 eV: use of new oscillator strengths of 0.5 per cent accuracy

M. Shallis, D. Blackwell, 1979 .

Precision measurement of relative oscillator strengths for Ti I – II. Transitions from levels ${a}^{5}{F}_{1-4}\,(0.81-0.84\,\text{eV}),\,{a}^{1}{D}_{2}\,(0.90\,\text{eV})\,\text{and}\,{a}^{3}{P}_{0-2}$(1.5-1.07 eV)

M. Shallis, D. Blackwell, A. Petford, 1982 .

Precision measurement of relative oscillator strengths for Ti I – I. Transitions from levels a3 F2 (0.00 eV) and a3 F3 (0.02 eV) and a3 F4 (0.05 eV) measured with an accuracy of 0.5 per cent

S. Leggett, M. Shallis, D. Blackwell, 1982 .

Analysis of Mn I lines in the solar spectrum using accurate oscillator strengths

M. Shallis, A. Booth, D. Blackwell, 1984 .

Measurement of relative oscillator strengths for Mn I. Transitions from levels in the range 0 eV < χ < ∼ 3 eV

M. Shallis, A. Booth, D. Blackwell, 1984 .

Hyperfine structure measurements for lines of astrophysical interest in Mn I

M. Shallis, A. Booth, M. Wells, 1983 .

Stellar angular diameters from infrared photometry. Application to Arcturus and other stars; with effective temperatures.

M. J. Shallis, D. E. Blackwell, M. Shallis, 1977 .

The infrared flux method for determining stellar angular diameters and effective temperatures

M. J. Selby, M. J. Shallis, D. E. Blackwell, 1979 .

Close Encounters?: Science and Science Fiction

M. Shallis, M. Shortland, A. Swift, 1990 .

Measurement of the absolute flux from Vega in the K band (2.2 µm)

M. Shallis, D. Blackwell, A. Petford, 1980 .

Precision measurement of relative oscillator strengths – IV. Attainment of 0.5 per cent accuracy. Fe I transitions from levels a5 D0−4 (0.00−0.12 eV)

P. Ibbetson, M. Shallis, D. Blackwell, 1979 .

Young People's Image of the Scientist.

P. Hills, M. Shallis, 1975 .

Where Is Silicon Culture

S. Turkle, E. Rogers, J. K. Larsen, 1986 .

Use of the infra-red flux method for determining stellar effective temperatures and angular diameters; the stellar temperature scale.

M. Shallis, D. Blackwell, A. Petford, 1980 .

Precision measurement of relative oscillator strengths – VII. Comparison between measured lifetimes of excited Fe I levels and values calculated from precise oscillator strengths

M. Shallis, D. Blackwell, 1979 .

Note on the interpretation of Fe I lines (2.18–2.49 eV) in the solar spectrum

G. J. Simmons, M. Shallis, D. Blackwell, 1982 .